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<ead xmlns="urn:isbn:1-931666-22-9" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="urn:isbn:1-931666-22-9 http://www.loc.gov/ead/ead.xsd"><eadheader countryencoding="iso3166-1" dateencoding="iso8601" langencoding="iso639-2b" repositoryencoding="iso15511"><eadid countrycode="US" mainagencycode="US-NNC-RB" url="http://findingaids.cul.columbia.edu/ead/nnc-rb/ldpd_5490814"></eadid><filedesc><titlestmt><titleproper>Kevin H. Prendergast papers <num>5490814</num></titleproper></titlestmt><publicationstmt><publisher>Rare Book and Manuscript Library</publisher><address><addressline>Butler Library, 6th Floor</addressline><addressline>Columbia University, Mail Code 1127</addressline><addressline>535 W. 114th St.</addressline><addressline>New York, NY 10027</addressline><addressline>Business Number: (212) 854-5153</addressline><addressline>Fax Number: (212) 854-1365</addressline><addressline>rbml@libraries.cul.columbia.edu</addressline><addressline>URL: <extptr xlink:href="http://www.columbia.edu/cu/lweb/indiv/rbml/index.html" xlink:show="new" xlink:title="http://www.columbia.edu/cu/lweb/indiv/rbml/index.html" xlink:type="simple"/></addressline></address><p>This finding aid is made available for public use following the Universal 1.0 Public Domain Dedication Creative Commons designation.</p></publicationstmt><notestmt><note><p>Contents list, 13 pagesFolder level control</p></note></notestmt></filedesc><profiledesc><creation>This finding aid was produced using ArchivesSpace on <date>2024-01-10 11:32:59 -0500</date>.</creation><langusage>Description is written in: <language langcode="eng" scriptcode="Latn">English, Latin script</language>.</langusage></profiledesc><revisiondesc><change><date>2010-02-24</date><item>Legacy finding aid created from Pro Cite.</item></change><change><date>2019-05-20</date><item>EAD was imported spring 2019 as part of the ArchivesSpace Phase II migration.</item></change></revisiondesc></eadheader><archdesc level="collection">
  <did>
    <repository>
      <corpname>Rare Book and Manuscript Library</corpname>
    </repository>
    <unittitle>Kevin H. Prendergast papers</unittitle>
    <origination label="Creator">
      <persname source="ingest">Prendergast, Kevin H., 1929-2004</persname>
    </origination>
    <unitid>5490814</unitid>
    <unitid>MS#1023</unitid>
    <langmaterial>
      <language langcode="eng" scriptcode="Latn">English</language>
.    </langmaterial>
    <physdesc altrender="whole">
      <extent altrender="materialtype spaceoccupied">20 linear feet</extent>
      <extent altrender="carrier">48 boxes</extent>
    </physdesc>
    <unitdate datechar="creation" normal="1954/1990" type="inclusive">1954-1990</unitdate>
  </did>
  <arrangement id="aspace_5ad01d98f74284e0565f1f6467002454">
    <head>Arrangement</head>
<p>This collection is arranged into 12 series.</p>  </arrangement>
  <accessrestrict id="aspace_6a95271bdeffc795fd3efe65e9f0d517">
    <head>Restrictions on Access</head>
<p>This collection is located off-site. You will need to request this material at least three business days in advance to use the collection in the Rare Book and Manuscript Library reading room.</p>  </accessrestrict>
  <accessrestrict id="aspace_6b9c7891aab9ec3d12a13cab2be1f506">
    <head>Restrictions on Access</head>
<p>This collection has no restrictions.</p>  </accessrestrict>
  <scopecontent id="aspace_c0b5db07e8e8492fd37950f3d9428ac4">
    <head>Summary</head>
<p>Correspondence, manuscripts, lectures, notes, and printed materials of Kevin H. Prendergast, a prominent astronomer who worked in the fields off dynamics of many-body systems, the rotation curves of galaxies, and X-ray binary systems.</p>  </scopecontent>
  <prefercite id="aspace_443ff3e0ca31aa8bc9c609017d6b05ed">
    <head>Preferred Citation</head>
<p>Identification of specific item; Date (if known); Kevin H. Prendergast papers; Box and Folder; Rare Book and Manuscript Library, Columbia University Library.</p>  </prefercite>
  <userestrict id="aspace_4a38389a287fb126299b540c3ffd2318">
    <head>Terms Governing Use and Reproduction</head>
<p>Reproductions may be made for research purposes. The RBML maintains ownership of the physical material only. Copyright remains with the creator and his/her heirs. The responsibility to secure copyright permission rests with the patron.</p>  </userestrict>
  <acqinfo id="aspace_36161bb02dd908d58541da208563dbbe">
    <head>Immediate Source of Acquisition</head>
<p>2004-2005-M35: Source of acquisition--Jane Prendergast. Method of acquisition--Gift; Date of acquisition--2/1/2005.</p>  </acqinfo>
  <bioghist id="aspace_07182e891a0e33bff0c97b5e4953917c">
    <head>Biographical / Historical</head>
<p>Prendergast received his Ph.D. at Columbia in 1954 and then went to the University of Chicago, returning to Columbia as a professor in 1962. He chaired the Columbia astronomy department from 1978 to 1984, retiring in 2000 with a long trail of successful young theorists in his wake. Prendergast was an icon in the field of dynamics of many-body systems. He also was well known for a series of papers in the 1960s and 1970s, written with Geoffrey and Margaret Burbidge, on understanding the rotation curves of galaxies. Numerous theoretical studies of the structure of galaxies followed, and he was a pioneer in the study of X-ray binary systems. In addition to Prendergast's professional accomplishments, he was also a skilled pianist and an avid sailor. During his long career, Prendergast became famous for using yellow legal pads, on which he had scrawled analyses of many problems in astronomical dynamics. His classes were renowned for the exactitude of his standards and the high percentage of faculty in attendance. During one year, regularly attending faculty outnumbered students.</p>  </bioghist>
  <processinfo id="aspace_a39ee25dd86974388ed9050a79a1bbf2">
    <head>Processing Information</head>
<p>Papers processed Wei-Hwan Chiang 10/2005.</p>  </processinfo>
  <accruals id="aspace_5284f706f4c49c02057fcd6491b2be6b">
    <head>Accruals</head>
<p>Materials may have been added to the collection since this finding aid was prepared. Contact rbml@columbia.edu for more information.</p>  </accruals>
  <controlaccess>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh85033169" source="lcsh">Cosmology</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh94002242" source="lcsh">X-ray binaries</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh2003009310" source="lcsh">Barred galaxies -- Rotation</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh2003009304" source="lcsh">Galactic dynamics</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh94002744" source="lcsh">Stellar dynamics</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh2003009309" source="lcsh">Spiral galaxies -- Rotation</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh85040180" source="lcsh">Dwarf galaxies</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh85127422" source="lcsh">Stars -- Clusters</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh85148743" source="lcsh">X-ray sources, Galactic -- Accretion</subject>
    <subject authfilenumber="http://id.loc.gov/authorities/subjects/sh85102674" source="lcsh">Asteroids</subject>
    <corpname authfilenumber="http://id.loc.gov/authorities/names/no95039994" source="naf">Columbia University. Department of Astronomy</corpname>
  </controlaccess>
  <dsc><c id="aspace_ae631dfc6bfa4c2b2c3874aadee6d56d" level="series"><did><unittitle>Series I: Personal</unittitle></did><c id="aspace_3da55172ddda3793b0440220e500047d" level="subseries"><did><unittitle>Subseries I.1: Photography</unittitle></did><c id="aspace_d78444fc568386d86268ede68644d694" level="file"><did><unittitle>Photograph (1)</unittitle><container id="aspace_0b4461bcd6e458ff6278304781d9bd35" label="box [RS00777412]" type="box">1</container></did></c></c><c id="aspace_c5247612b8188684652d108171be3b83" level="subseries"><did><unittitle>Subseries 1.2: Correspondence</unittitle></did><c id="aspace_68e22ba88535d381f039da39b5a03206" level="file"><did><unittitle>Chandra</unittitle><container id="aspace_21908e02ecf2c28036046039d19070c9" label="box [RS00777412]" type="box">1</container></did></c><c id="aspace_0cf0ff9f48cf6a48583882657c7e5312" level="file"><did><unittitle>Contopolous</unittitle><container id="aspace_e735f19549b89f6f351f02a88583f390" label="box [RS00777412]" type="box">1</container></did></c><c id="aspace_eb57fa41395c3a218027185366d5a7bc" level="file"><did><unittitle>Penthame</unittitle><container id="aspace_c53a0bf2c00342fd165a5c9626710d20" label="box [RS00777412]" type="box">1</container></did></c><c id="aspace_47e7f86745b96c0c638cd6add8c6531d" level="file"><did><unittitle>Pesch, Peter</unittitle><container id="aspace_60ed6d023714a2d673b20af6cca3dde1" label="box [RS00777412]" type="box">1</container></did></c><c id="aspace_83e996c2800e6b64d94b48671ae1c9ba" level="file"><did><unittitle>Slyz, Adrianne</unittitle><container id="aspace_e9075233d52f69595b3cc234cf6c1706" label="box [RS00777412]" type="box">1</container></did></c><c id="aspace_2d2d3d74d8c9b04def27ac8a0353fa51" level="file"><did><unittitle>Spiegel, Edward</unittitle><container id="aspace_78e068ddac80fb0d386d80ffb0cf6361" label="box [RS00777412]" type="box">1</container></did></c><c id="aspace_c9f7bf4df3a46ab0eb4fb2bd5d61912d" level="file"><did><unittitle>Xu, Kun</unittitle><container id="aspace_f2a0fce849b9924c0a9f0b8350fa646a" label="box [RS00777536]" type="box">2</container></did></c></c></c><c id="aspace_7b042f70c913afacd72d7bc16fa56638" level="series"><did><unittitle>Series II: Astronomy</unittitle></did><c id="aspace_191b191b6a472042c964fe3d5a5e9621" level="subseries"><did><unittitle>Subseries II.1: Cosmology</unittitle></did><c id="aspace_4c96067426e6ce6e8dfdcd5dd27d5261" level="file"><did><unittitle>Equations about cosmology</unittitle><physdesc id="aspace_a518024a432dc83270bee1db3c6a2150">166 pages</physdesc><container id="aspace_106e918d1e9e5c7395d48d3e267eccb7" label="box [RS00777420]" type="box">3</container></did></c></c><c id="aspace_5392795bcc3058d8ab3f36deb7e8040f" level="subseries"><did><unittitle>Subseries II.2: Dynamics of Galaxies: General</unittitle></did><c id="aspace_cea6d862d7829bfc7aaeae95aeef263c" level="file"><did><unittitle>Galactic Dynamics</unittitle><container id="aspace_ccfb80a2348ffe0a96878ca94a50fbe1" label="box [RS00777420]" type="box">3</container></did></c><c id="aspace_7e6c5bcaaedd1d4b4d09950d0408a5e5" level="file"><did><unittitle>Gravitational slab problem</unittitle><container id="aspace_9fa8fdc51a16205bc8542b034963a386" label="box [RS00777420]" type="box">3</container></did></c><c id="aspace_9e91da17835441653f7be5a7c434d278" level="file"><did><unittitle>One-dimensional self-gravitating gas</unittitle><container id="aspace_763032e4dbc15b430649f02221988cf3" label="box [RS00777420]" type="box">3</container></did></c><c id="aspace_534dad6629f5c281e34032767dfdd4c2" level="file"><did><unittitle>Time dependent one-dimensional stellar system</unittitle><container id="aspace_0f15927aa8ddb0f1448fe2beb980ca12" label="box [RS00777420]" type="box">3</container></did></c><c id="aspace_56cb5347e862931e64fd64f752fcbd5f" level="file"><did><unittitle>Self consistent galaxy models (axisymmetric)</unittitle><container id="aspace_153a2151a986e3f7f33cae4cb462811b" label="box [RS00777420]" type="box">3</container></did></c><c id="aspace_7adf5d7c0dc0466dbdbbcabda7252a2d" level="file"><did><unittitle>Instability of rings (of mass)</unittitle><container id="aspace_7f8a02ca0929cbeff5bed8d8ccdcde93" label="box [RS00777544]" type="box">4</container></did></c><c id="aspace_8ed714d4c04627fdfe66c49ec1b6068b" level="file"><did><unittitle>Computer simulation of galactic evolution</unittitle><container id="aspace_adb2921b32bd6095386ab24d586e7066" label="box [RS00777544]" type="box">4</container></did></c><c id="aspace_c6508c9ad5d13610c77fbd8ccebfdf0d" level="file"><did><unittitle>Stochastic star formation in disk galaxies (mathematical description of a game theory)</unittitle><container id="aspace_f13ec9467b0a17ded2b8d16d54a338f7" label="box [RS00777544]" type="box">4</container></did></c><c id="aspace_c844e607a4f96bad2d299af341f19dd6" level="file"><did><unittitle>Stellar dynamics with star formation</unittitle><container id="aspace_298d327513d072070f6fdf21c5ac7f0f" label="box [RS00777544]" type="box">4</container></did></c><c id="aspace_02e21d7e53485484439230396056f0d0" level="file"><did><unittitle>"Oseen" approximation based on streamlines, etc.</unittitle><container id="aspace_0ebdf984de5d34b6866abfa572b3ecfe" label="box [RS00777544]" type="box">4</container></did></c><c id="aspace_0f5c5e9125cc66387c6226a8043357bf" level="file"><did><unittitle>Theoretical studies of M101</unittitle><container id="aspace_59b5db11fdd42b61922b4e536ebe0ccc" label="box [RS00777544]" type="box">4</container></did></c></c><c id="aspace_58b9ff339d8240f2de621882622824c1" level="subseries"><did><unittitle>Subseries II.3: Dynamics of Galaxies: Spiral Galaxies</unittitle></did><c id="aspace_a51232c44f26ef6ff1bd2afb8c3edb11" level="file"><did><unittitle>Linear spiral structure</unittitle><container id="aspace_1029640a5855606dbb3ee24588a4bb9e" label="box [RS00777439]" type="box">5</container></did></c><c id="aspace_495267bc4ad515db6e00cbf8d7f90fbe" level="file"><did><unittitle>Stability of spiral arm shocks</unittitle><container id="aspace_ce9df76f17a5888f0af02c155078eebd" label="box [RS00777439]" type="box">5</container></did></c><c id="aspace_9600d4914a101605cbf0ef3794cd208a" level="file"><did><unittitle>Thin gas disk: asymptotic theory of spiral arms (warped disk as finite system of coupled rings)</unittitle><container id="aspace_48cdf5c4780d9fd02c96550efe38e1c7" label="box [RS00777439]" type="box">5</container></did></c><c id="aspace_77d817e981787a07f4499d306346381b" level="file"><did><unittitle>Spiral Arm Problems: Linblad Resonance</unittitle><container id="aspace_475b5b6d6d0fb2c1f91dd7c02b8a1921" label="box [RS00777439]" type="box">5</container></did></c></c><c id="aspace_ee324cba1ba80aea7985ab6dd95b98ac" level="subseries"><did><unittitle>Subseries II.4: Dynamics of Galaxies: Barred Spiral Galaxies</unittitle></did><c id="aspace_efcdecca9ef61bba29dcbf98c4e31c96" level="file"><did><unittitle>Barred Spirals</unittitle><unitdate datechar="creation">[1974?]</unitdate><container id="aspace_286fd31ddab483329469b672b79f20bb" label="box [RS00777439]" type="box">5</container></did></c><c id="aspace_58c4959cd5a10017f5c02912b7f72683" level="file"><did><unittitle>Barred Spirals</unittitle><container id="aspace_fb05e8fe88d3372f63be71afa0685663" label="box [RS00777439]" type="box">5</container></did></c><c id="aspace_0a5351817fafa032cefaf136ad66212f" level="file"><did><unittitle>Barred spiral galaxies (I, II, III, IV, V, VI, VII, VIII)</unittitle><unitdate datechar="creation">(1960s, 1970s)</unitdate><container id="aspace_787fb6cf7accae9ff4ca2448c4997abd" label="box [RS00777552]" type="box">6</container></did></c><c id="aspace_66705c9d7f14cf908c7ca8ceedb3d9ed" level="file"><did><unittitle>Barred spiral galaxies—some plots &amp; shock waves in barred spiral galaxies</unittitle><container id="aspace_260be5c7bcf8e59f945546fd7f911c7a" label="box [RS00777552]" type="box">6</container></did></c><c id="aspace_94f4b3480cce18610112526578e0a1bf" level="file"><did><unittitle>Barred spirals Roche modes</unittitle><container id="aspace_8d5b7ab66d88d730c976c9d1360b26a5" label="box [RS00777552]" type="box">6</container></did></c><c id="aspace_6807bf6c1945c941803660c47a33ed44" level="file"><did><unittitle>Gradient wind approximation</unittitle><container id="aspace_317e748c9bd03c6ad133d204467a9a2c" label="box [RS00777552]" type="box">6</container></did></c><c id="aspace_feaf2dbf733f678cfa9e0bbd4d1c166c" level="file"><did><unittitle>Potential of oblate spheroid</unittitle><container id="aspace_33ff4fa7c4ad83398328833291e6aa33" label="box [RS00777552]" type="box">6</container></did></c><c id="aspace_5bfac0cf82644fa0578121d8ca27ab38" level="file"><did><unittitle>Symmetry properties</unittitle><container id="aspace_c4aaeacecdf8a9be93d66ab408bc4d8f" label="box [RS00777552]" type="box">6</container></did></c><c id="aspace_e9402b364d9413ba8485d676ccf74328" level="file"><did><unittitle>Theoretical studies of gas flow in barred spiral galaxies</unittitle><container id="aspace_63eb438ba97e37987e31fe57a90bfeba" label="box [RS00777447]" type="box">7</container></did></c><c id="aspace_61f8a50636cf0b642f307d3b0058ceef" level="file"><did><unittitle>Barred spiral shocks</unittitle><container id="aspace_c73d97ac0bf0548f5621685e0a3ff68b" label="box [RS00777447]" type="box">7</container></did></c><c id="aspace_4cbd234ffde231a6c08f3a8c1ee856c3" level="file"><did><unittitle>Barred spiral galaxies: material for a talk based on a paper on "Theoretical studies of gas flows in barred spiral galaxies" by K. Prendergast</unittitle><container id="aspace_ec3e14a26c05e78edca7aae565521479" label="box [RS00777447]" type="box">7</container></did></c><c id="aspace_185679b98af274dd79e05e2911fd03d5" level="file"><did><unittitle>Barred spiral galaxies [talk], Yale</unittitle><unitdate datechar="creation">1978</unitdate><container id="aspace_2f96126d536f87576092b8a16c650fbd" label="box [RS00777447]" type="box">7</container></did></c><c id="aspace_06736b8d6b7ba62e685093be3c111121" level="file"><did><unittitle>Talk given by Kevin Prendergast on barred spiral galaxies</unittitle><unitdate datechar="creation">1982</unitdate><container id="aspace_0af0285569d46dc5d91bd3ab0d327ff8" label="box [RS00777447]" type="box">7</container></did></c></c><c id="aspace_c5678aaa17999e4da76cc86da63a4d64" level="subseries"><did><unittitle>Subseries II.5: Dynamics of Galaxies: Dwarf Elliptical Galaxies (and Elliptical Galaxies)</unittitle></did><c id="aspace_e80fa9769389f552ad11f4c56bc5f995" level="file"><did><unittitle>Dwarf elliptical galaxies--analytical approximation (two-fluid with gravity)</unittitle><container id="aspace_1a9ae4f017ba51e3c905252e1ebe2bd3" label="box [RS00777447]" type="box">7</container></did></c><c id="aspace_feb80cbf2b190889430c830b7273b39d" level="file"><did><unittitle>Two-fluid spherical models</unittitle><container id="aspace_c5e5d8bb4fd218e80f3f4d4dea2750a9" label="box [RS00777560]" type="box">8</container></did></c><c id="aspace_dc455f361990e8548a60d1b5d34e71b3" level="file"><did><unittitle>Analytic approximation, two-fluid with gravity</unittitle><container id="aspace_76bbb1cf96df230c5de3ca3e6391d359" label="box [RS00777560]" type="box">8</container></did></c><c id="aspace_493da4362c884aadbd65cc89bdd13a5a" level="file"><did><unittitle>Modeling the formation of elliptical and dwarf galaxies using a spheroidal two-fluid system with self-gravity</unittitle><container id="aspace_d7af0ebb54363c2135aa383a073a0153" label="box [RS00777560]" type="box">8</container></did></c><c id="aspace_e2fcadfc18242ccb2e3b8fa96fa48763" level="file"><did><unittitle>Numerical Simulations of the Formation of Dwarf Ellipticals (I,II, III, IV, V)</unittitle><container id="aspace_07ce6e00b54523e7a95bb4386e7bc8c0" label="box [RS00777560]" type="box">8</container></did></c><c id="aspace_2cc026f278e953f39263141c9e486a62" level="file"><did><unittitle>Marseille collaboration papers (published)</unittitle><container id="aspace_a4b8492477eaf370598fc1fa0c127027" label="box [RS00777560]" type="box">8</container></did></c><c id="aspace_efd852bf62f430d4d01f2e64db04a30e" level="file"><did><unittitle>Marseille</unittitle><container id="aspace_5830e7b3840066333b16cbd31bb4479f" label="box [RS00777455]" type="box">9</container></did></c><c id="aspace_f44b6237161333d45f3fc2d10d490561" level="file"><did><unittitle>Marseille</unittitle><container id="aspace_970027f24449aa3e0959d2af74aa8c75" label="box [RS00777579]" type="box">10</container></did></c><c id="aspace_39e4d60ae51403024feb17e66d838c7a" level="file"><did><unittitle>Marseille</unittitle><container id="aspace_767f283c4278b24dff233b3639819af0" label="box [RS00777463]" type="box">11</container></did></c><c id="aspace_3d6bb17663909367f6d9e2b0d7512c72" level="file"><did><unittitle>Marseille</unittitle><container id="aspace_0b18a741140b6d7b77245ca839f8ee81" label="box [RS00777587]" type="box">12</container></did></c><c id="aspace_1d58bf6111d2ce677c98746b8ff4775b" level="file"><did><unittitle>Marseille</unittitle><container id="aspace_fcefa3a3fd5ddeae95922c55289683fe" label="box [RS00777471]" type="box">13</container></did></c><c id="aspace_dc369f9bdcd72ce00dab381bbbcbca94" level="file"><did><unittitle>Marseille numerical simulation results and some theoretical analysis of those models</unittitle><container id="aspace_3938cba1f0cbb071286afe3b1973eba8" label="box [RS00777595]" type="box">14</container></did></c><c id="aspace_c83262fe4ff636f3407cf50e1e6d0927" level="file"><did><unittitle>Marseille numerical simulations</unittitle><container id="aspace_4c3effaea687bc0d1d78a83e6998838b" label="box [RS00777480]" type="box">15</container></did></c><c id="aspace_1df1475bdc3e53d7ac9e294a04411e02" level="file"><did><unittitle>Marseille numerical simulations</unittitle><container id="aspace_1a2f1584dc2ff4b58f795e2909eb88a0" label="box [RS00777609]" type="box">16</container></did></c><c id="aspace_06c029af28f5a21b8c67326602a5cfdc" level="file"><did><unittitle>Marseille numerical simulations</unittitle><container id="aspace_cf6df535c614827c4964e2fd510a70ba" label="box [RS00777498]" type="box">17</container></did></c><c id="aspace_5d75e40205b99ee87a487b1216d204d1" level="file"><did><unittitle>Marseille numerical simulation results performed at Marseille Observatory, France (collaborators Lia Athanassoula et al.)</unittitle><unitdate datechar="creation">1988</unitdate><container id="aspace_96e1f893fd1333a96b0d82df0dab32d4" label="box [RS00777617]" type="box">18</container></did></c><c id="aspace_4ba9f100a4a67d3aa0a160b3112d3767" level="file"><did><unittitle>Numerical models (including programs) and results for one-dimensional two-fluid (Cartesian grid) and Marseille models</unittitle><container id="aspace_469ff9677207e044edc52e25fd733304" label="box [RS00777617]" type="box">18</container></did></c><c id="aspace_04c6f5eb9b8ec068b68910c2dd93acc3" level="file"><did><unittitle>Dwarf galaxies formation models (Marseille 1994) and other numerical modeling results (including programs)</unittitle><container id="aspace_b6293c2cc8d629b1c26413aca68d2b9d" label="box [RS00777617]" type="box">18</container></did></c><c id="aspace_5e28de82b2b51899bca380cadd875e3e" level="file"><did><unittitle>Various numerical simulation results of the Marseille collaboration [mostly in the form of diagrams]</unittitle><container id="aspace_8fec56587b6d704336ea29859f826844" label="box [RS00777501]" type="box">19</container></did></c><c id="aspace_cf4ddc50755c500e8b899bf541f38152" level="file"><did><unittitle>Marseille Observatory simulation results used for Columbia Astrofest talk</unittitle><unitdate datechar="creation">1996</unitdate><container id="aspace_ad5775c867b5acf3e5b0d652330a7d31" label="box [RS00777501]" type="box">19</container></did></c><c id="aspace_b439201b3273fd0e8b22cf407e1d7b68" level="file"><did><unittitle>Dwarf elliptical galaxy formation, talk given at Columbia</unittitle><unitdate datechar="creation">1990</unitdate><container id="aspace_01b60cab020ad21a3e7ff8bae88aa607" label="box [RS00777501]" type="box">19</container></did></c></c><c id="aspace_2f24f5ecc2d47b346756c2645b5554f3" level="subseries"><did><unittitle>Subseries II.6: Dynamics of Galaxies: Star-Gas Interactions in Galaxies</unittitle></did><c id="aspace_cd282c31edbedeaabd8915a29ff91031" level="file"><did><unittitle>Two-fluid (stars and gas) linear stability analysis</unittitle><unitdate datechar="creation">1980</unitdate><container id="aspace_51ee19f4bac5ef3895be0f568ff44952" label="box [RS00777501]" type="box">19</container></did></c><c id="aspace_9a3efd44e602ec503f8099ff90465d0a" level="file"><did><unittitle>Two-fluid hydrodynamic model</unittitle><unitdate datechar="creation">1978</unitdate><container id="aspace_fabc5a96733457258a4b3b55d1450546" label="box [RS00777501]" type="box">19</container></did></c><c id="aspace_892a0a8c4ef53a5c41470e838c9d590a" level="file"><did><unittitle>3-fluid model (gas, high mass star, low mass star)</unittitle><container id="aspace_32644c05b1ccb205b0218d0db41c1821" label="box [RS00777501]" type="box">19</container></did></c><c id="aspace_0abf892e9841ef026ca8682982556c07" level="file"><did><unittitle>Two-fluid star-gas model [talk], Charlottesville, Virginia</unittitle><container id="aspace_f854be6f489d848ab6e3aff716cf6552" label="box [RS00777625]" type="box">20</container></did></c><c id="aspace_f486cfc44bea2721658784aa954e647d" level="file"><did><unittitle>Talk given at European Southern Observatory, Munich, Germany</unittitle><container id="aspace_f29d8b4c6e5606ddd8bceb4b3782640d" label="box [RS00777501]" type="box">19</container></did></c></c><c id="aspace_19445d6a8afbb9e5f91bee33ac7157a9" level="subseries"><did><unittitle>Subseries II.7: Star Clusters</unittitle></did><c id="aspace_f8a7352f6c4dcfd76574a892957e29a3" level="file"><did><unittitle>Escape of stars from clusters: statistical mechanical approach</unittitle><unitdate datechar="creation">1980s</unitdate><container id="aspace_53a5ac4e75dcc40f44c0a65332c03ad4" label="box [RS00777625]" type="box">20</container></did></c></c><c id="aspace_7279a3ee9a7e94c90e343a5ddba40e29" level="subseries"><did><unittitle>Subseries II.8: Accretion Disks</unittitle></did><c id="aspace_1a434a958357ab13d52c7623769d3b4d" level="file"><did><unittitle>X-ray generation in accretion disk in binary systems, gas streams in close binary systems</unittitle><container id="aspace_e574e6572c25f90bf6c78b2b6f026b11" label="box [RS00777625]" type="box">20</container></did></c><c id="aspace_d67262e34663e6e14e99d6de14cda0a6" level="file"><did><unittitle>Binary Stellar Systems</unittitle><container id="aspace_923794649a5a5bf05055fb056e2332a3" label="box [RS00777625]" type="box">20</container></did></c></c><c id="aspace_e70ffd444ce869fe1642c9a093b98055" level="subseries"><did><unittitle>Subseries II.9: Asteroid</unittitle></did><c id="aspace_a406f954f3f165f460ffb2163941f9ba" level="file"><did><unittitle>Asteroid</unittitle><unitdate datechar="creation">1950s</unitdate><container id="aspace_75813c0ea6d5de6317c55fed5d2d0b17" label="box [RS00777510]" type="box">21</container></did></c><c id="aspace_d66d05a02b5e9033d2b9d4704f58dcb3" level="file"><did><unittitle>Rotating asteroid</unittitle><unitdate datechar="creation">1950s</unitdate><container id="aspace_7dd9e33fbb66e4477abd9736a7362f2a" label="box [RS00777510]" type="box">21</container></did></c><c id="aspace_bf275ecf423f71fdd385fa0b1772f2ba" level="file"><did><unittitle>Rotating asteroid (I, II, III, IV, V)</unittitle><unitdate datechar="creation">1950</unitdate><container id="aspace_99e5a4cd8abd1821177e96a00316485c" label="box [RS00777510]" type="box">21</container></did></c></c><c id="aspace_fc19bbeeeb6e3ee681dc766badae2bbe" level="subseries"><did><unittitle>Subseries II.10: Few- and N-body Problems, and Celestial Mechanics</unittitle></did><c id="aspace_04709065160e344d30ed5eff53206fce" level="file"><did><unittitle>Statistics of the gravitational three- and four-body problems</unittitle><container id="aspace_1baf1be6db38b219602b6d8029fa74d6" label="box [RS00777633]" type="box">22</container></did></c><c id="aspace_7fd8594f047cbf412b2ef8b6f6b8e6cb" level="file"><did><unittitle>Statistics of three-body problem</unittitle><container id="aspace_644ace1d01218620f599a93e5cf2f753" label="box [RS00777633]" type="box">22</container></did></c><c id="aspace_303a296b700227c6a48a7ba5879d33d7" level="file"><did><unittitle>N-body problem</unittitle><unitdate datechar="creation">1970</unitdate><container id="aspace_16610b9f88b2ef4233c28c7ab311d234" label="box [RS00777528]" type="box">23</container></did></c><c id="aspace_33a50298df0f228a8bee480991c399ed" level="file"><did><unittitle>Large N problems (N-particle systems)</unittitle><container id="aspace_eb5f69e9a794d20a949f317c71c2ce1b" label="box [RS00777528]" type="box">23</container></did></c><c id="aspace_2eb2da90cebd27dea7c21cdb880350a2" level="file"><did><unittitle>N-Body, NYU</unittitle><unitdate datechar="creation">1980</unitdate><container id="aspace_ea58a7e8cea70d6dbfce254cfe4b9dfa" label="box [RS00777528]" type="box">23</container></did></c><c id="aspace_1dca7a9914b72052699c0cd14c7ad86e" level="file"><did><unittitle>Celestial mechanics I</unittitle><container id="aspace_15d6d0272e973778ebd6e7869b08559b" label="box [RS00777528]" type="box">23</container></did></c><c id="aspace_a10e84cb6027d1a596e458c320f41264" level="file"><did><unittitle>Celestial mechanics II</unittitle><container id="aspace_a680dfceb351e8f9ef189d48cae53b1c" label="box [RS00777528]" type="box">23</container></did></c></c><c id="aspace_2c48d0c83312195537978c1deb3f7fcf" level="subseries"><did><unittitle>Subseries II.11: Hydrodynamics, Astrophysical Fluid Dynamics, and Gas-Kinetic Theory</unittitle></did><c id="aspace_62458b8ddb2427bb898743b21baf5210" level="file"><did><unittitle>A series of analytic studies (notebooks I-VI) on hydrodynamics, as moment equations of the Boltzmann equation</unittitle><container id="aspace_36027f5843466a866030fad195bf637c" label="box [RS00777641]" type="box">24</container></did></c><c id="aspace_70d93381d73c23cd30ec0c79b6970812" level="file"><did><unittitle>Singularities of one dimensional hydrodynamic system using pseudo Liouville equation</unittitle><container id="aspace_1145b2e1acc4dc493bea2d81f9cb623d" label="box [RS00777641]" type="box">24</container></did></c><c id="aspace_d221677b14a48a94d59bc934d26ccb1b" level="file"><did><unittitle>Gravity in the BGK scheme for hydrodynamics</unittitle><container id="aspace_558a747faa1debe309b89f85460a31de" label="box [RS00777641]" type="box">24</container></did></c><c id="aspace_f9c5a81c2b111093276f0118c4fbba98" level="file"><did><unittitle>Solution of the Krook equation at shock</unittitle><container id="aspace_ce73a64e48aa57bbf776b0eb683e048b" label="box [RS00777641]" type="box">24</container></did></c><c id="aspace_a982d701c1db70fb2ec7e9cc48a2d284" level="file"><did><unittitle>Collisional hydrodynamic scheme (CHS)—theoretical derivation of the method</unittitle><container id="aspace_08d619459f0bcf84fac79e2b0734b15d" label="box [RS00777641]" type="box">24</container></did></c><c id="aspace_c817d27f166530f9d537badfdda0c0dd" level="file"><did><unittitle>Radial flow</unittitle><container id="aspace_24ecf968956b83f309f3efe0b8b76bbd" label="box [RS00777650]" type="box">25</container></did></c><c id="aspace_2d51374605a97fbf3e5da3ac7fd4dd43" level="file"><did><unittitle>Wave-driven winds—several manuscripts</unittitle><container id="aspace_4967d710e140148d3a8e9036c2cc6104" label="box [RS00777650]" type="box">25</container></did></c><c id="aspace_64fee051f1e311a0fc252be366c328ca" level="file"><did><unittitle>Breaking waves</unittitle><unitdate datechar="creation">1984</unitdate><container id="aspace_ec71c875f0042c6bb125c23dde9d3f7f" label="box [RS00777650]" type="box">25</container></did></c><c id="aspace_3ed7512a19170c3f812c7e0063fcbd12" level="file"><did><unittitle>Nonlinear convection</unittitle><unitdate datechar="creation">[1980s?]</unitdate><container id="aspace_4cfc7d4ecd3642fbb8bb978d55156ecb" label="box [RS00777650]" type="box">25</container></did></c><c id="aspace_18a1b2efea2c525fc91cc6096f68c461" level="file"><did><unittitle>Nonlinear convection—rational approximation</unittitle><unitdate datechar="creation">[1981?]</unitdate><container id="aspace_9cb22ca43ba08f422d43659cd40bba38" label="box [RS00777650]" type="box">25</container></did></c><c id="aspace_b86b32f3556817c5a66fbf23a8de3a92" level="file"><did><unittitle>Turbulence sphere</unittitle><unitdate datechar="creation">1970s</unitdate><container id="aspace_5e47c3e9f710197d39efdb5512de44c1" label="box [RS00777650]" type="box">25</container></did></c><c id="aspace_a777da1c6209abe7b77f775930abc8b7" level="file"><did><unittitle>Angular momentum (of turbulent fluid)</unittitle><container id="aspace_bf7bafde80c4711f2b45bfb66bba1ab3" label="box [RS00777668]" type="box">26</container></did></c><c id="aspace_f01132e009d18f8242f8d858fcbb01f3" level="file"><did><unittitle>Hydrodynamics—variational principle</unittitle><container id="aspace_1513ec703f6cf61be778152d0c4fcc0a" label="box [RS00777668]" type="box">26</container></did></c><c id="aspace_e98701b05c5e9fd9f7ff66e0a7c7d5dd" level="file"><did><unittitle>Burger's equation</unittitle><container id="aspace_2a054141bea2a757045a62d86fe9c1ba" label="box [RS00777668]" type="box">26</container></did></c><c id="aspace_87b8e65d13f550493ee09c8fa2650bdd" level="file"><did><unittitle>Burger's equation—singularities (inviscid)</unittitle><container id="aspace_ac6e94989a6fc6b73a82898d120d84f7" label="box [RS00777668]" type="box">26</container></did></c><c id="aspace_5c0930ab4bf293350488e3a4864ea6d2" level="file"><did><unittitle>Burger's equation—two-dimensional inviscid</unittitle><container id="aspace_521b6c9398ba825c1edd0099a8aa36cf" label="box [RS00777668]" type="box">26</container></did></c><c id="aspace_d565106eed9ce02b2702e19085bab89a" level="file"><did><unittitle>Burger's equation with viscosity and potential</unittitle><container id="aspace_b491c5ec0821d62e5cd85b1ac6c339d6" label="box [RS00777676]" type="box">27</container></did></c><c id="aspace_3c0f6b48b0dd1bbebd4efd80c820df8d" level="file"><did><unittitle>Burger's equation (two-dimensional inviscid)—singularities (talk given at Columbia)</unittitle><container id="aspace_f41ed9bd1a365ae763af7f820b553b93" label="box [RS00777676]" type="box">27</container></did></c><c id="aspace_7f7f1fe21d475f4d4ed2a93fc749591d" level="file"><did><unittitle>Gas Kinetic Theory in General (including Radiative Transfer)</unittitle><container id="aspace_44a781705815d5e9a865a104d35aab32" label="box [RS00777676]" type="box">27</container></did></c><c id="aspace_6dd721ef564d2dd9bcc8ff4940895c9b" level="file"><did><unittitle>Hydrodynamics in General</unittitle><container id="aspace_0f435c14938c3bdf420174d878d4d573" label="box [RS00777676]" type="box">27</container></did></c></c><c id="aspace_a7fba36a7a25f5194b04650e1fd89b4c" level="subseries"><did><unittitle>Subseries II.12: Magnetohydrodynamics</unittitle></did><c id="aspace_b69069bb308308df7ca4091117abf260" level="file"><did><unittitle>Hydromagnetic similarity solutions I</unittitle><unitdate datechar="creation">1975</unitdate><container id="aspace_d4aba3340eef766732a6412905845a0f" label="box [RS00777676]" type="box">27</container></did></c><c id="aspace_e2166a0268ec18a091e525f2cfb60116" level="file"><did><unittitle>Hydromagnetic similarity solutions II</unittitle><container id="aspace_26e508e5679d6093e45a205eeb0a3844" label="box [RS00777676]" type="box">27</container></did></c><c id="aspace_dad0ca58a889d5e954b95e0c3257a224" level="file"><did><unittitle>Axisymmetric time-dependent self-similar force-free fields</unittitle><container id="aspace_fd9b6363090eeb73a4ddf8330bababb2" label="box [RS00777676]" type="box">27</container></did></c><c id="aspace_77922dbd982fa3b96c792d02ca3bde7c" level="file"><did><unittitle>Force-free fields (axisymmetric)</unittitle><container id="aspace_1fab525ed225f0f61ed6ebadc62e0e74" label="box [RS00777676]" type="box">27</container></did></c></c></c><c id="aspace_a9cf114c2389fe8cfe5a759adf8aa33f" level="series"><did><unittitle>Series III: Dynamical Systems and Applied Mathematics</unittitle></did><c id="aspace_1018d3486b0cae1f92695dfa7105da70" level="file"><did><unittitle>Hamiltonian system (H=1⁄2(X.2+Y.2+X2+Y2)+X2Y)</unittitle><container id="aspace_f61c3a680e68332826296b6f8fcbc4c3" label="box [RS00777684]" type="box">28</container></did></c><c id="aspace_e5a9a5c3893e4e572966b332a7df55bf" level="file"><did><unittitle>Variational principle for Hamiltonian systems and vanishing Henyey determinant</unittitle><unitdate datechar="creation">[1980s?]</unitdate><container id="aspace_ba9420def4759226dfe971a5bbeeb175" label="box [RS00777684]" type="box">28</container></did></c><c id="aspace_cf3413494d118afbb780125f5848158b" level="file"><did><unittitle>Duffing equation</unittitle><container id="aspace_6469835aea6200f85ea9d4926981763d" label="box [RS00777684]" type="box">28</container></did></c><c id="aspace_a6e6ab4c48bd5248819e35c5c24a87b9" level="file"><did><unittitle>Duffing with driving</unittitle><container id="aspace_2c86f23df8b85e75b0bf39010e423b31" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_a3981707e12c946130f848ebb3fa363f" level="file"><did><unittitle>Duffing equation: NR correction</unittitle><container id="aspace_40bf4e335740df5ccb9fd11a9691d0ae" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_974d0b9b8dd43d05f6afacd1a50c0250" level="file"><did><unittitle>Duffing, van der Pol—high order approximation (rational approximation</unittitle><unitdate datechar="creation">[1980s?]</unitdate><container id="aspace_95814a467a5815835ee843df0ce3fc7d" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_033111a7131c5a058322093f3e93b813" level="file"><did><unittitle>Van der Pol oscillator</unittitle><unitdate datechar="creation">[1980s?]</unitdate><container id="aspace_273f35f459b5cb44e3e3acb6c4450f91" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_a45350eb3daaf6412abc73944a75867f" level="file"><did><unittitle>Van der Pol oscillator</unittitle><container id="aspace_5739e458b896dd50677e78ca437172ed" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_85a2738681f485ad96d23f8e5c3c369f" level="file"><did><unittitle>Hamilton-Jacobi equation</unittitle><container id="aspace_b30c1938877c86ae42b7df099dea6759" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_883345298da3cece841012f3e278b942" level="file"><did><unittitle>Fourier-Pade (x..+x7=0), higher order correction</unittitle><container id="aspace_cdaf57287c47304c150b2fe2752b3e37" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_6ddfc7080bb49257d50bdcba8b4d23f7" level="file"><did><unittitle>Fourier-Pade equation</unittitle><container id="aspace_3216ac5e6cc92f849a87fa88e330ba6e" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_38b9a5cf8c305c8500c4770cadfe345c" level="file"><did><unittitle>Fourier Pade equation ( (x..+x3=0), higher order correction</unittitle><container id="aspace_fda260405fcdd5459bb0d67ea1051df4" label="box [RS00777692]" type="box">29</container></did></c><c id="aspace_ef7f349249799503fb869a11086dbf1e" level="file"><did><unittitle>Fourier-Pade integration</unittitle><container id="aspace_34ef3a491778cdbb9c670ea379d773c1" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_98ee81245382dff0fd50d39b98b2cdc9" level="file"><did><unittitle>Pade: 2D: ordinary differential equations of higher order, 1D: quadratic, etc.</unittitle><container id="aspace_de0cb511ef0a9124e1660602ace097e5" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_90af18dad1b1ca79d27152a7b0f199a9" level="file"><did><unittitle>Mathieu equation</unittitle><container id="aspace_ad8cab7a2f60517e192b1e8d049b1f39" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_6fcd4b04745274dacc8fc81c25df773b" level="file"><did><unittitle>Mathieu equation: two-point approximation</unittitle><container id="aspace_32bf4f59913dd670c6049ab56ab0ab34" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_b6f67beb268873ea2729200c606a960a" level="file"><did><unittitle>kdV equation with implicit function</unittitle><container id="aspace_9a8b7fdf423085af01c99d7978200ade" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_f3bf7f90c170d679aeadb3e314a72768" level="file"><did><unittitle>Liouville equation</unittitle><container id="aspace_1d022c244407855187851a68dec93f89" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_2a2f93ace576d39116401ce24eaee465" level="file"><did><unittitle>Liouville equation (Woods Hole)</unittitle><unitdate datechar="creation">1969</unitdate><container id="aspace_008604ad80b5c7143d50b31b77f5374f" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_eb445b30a4aae16a150e393628b4bf4d" level="file"><did><unittitle>Eckonal equation</unittitle><container id="aspace_c7ff0edac2904561a421fbe47875ca19" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_599d814d6a90cbfb39c7aebe7542ab59" level="file"><did><unittitle>Rational approximation near w=0 (potential maximum)</unittitle><container id="aspace_deb129da0d0adcd07739fa7f4b07adea" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_94565db677a0ec77d7bc4bdec1edfed7" level="file"><did><unittitle>Rational-function orbits</unittitle><container id="aspace_016c1a850cb6dcfdafd308a2e62743a5" label="box [RS00777706]" type="box">30</container></did></c><c id="aspace_3df5e6cfe6e5ae74d1328b9c2c0c6b3c" level="file"><did><unittitle>Rational approximation for a Hamiltonian system</unittitle><container id="aspace_561da081f9203e97b8e97eb9b4fc52b2" label="box [RS00777714]" type="box">31</container></did></c><c id="aspace_668d1acd2fd596a93d69d411e25220aa" level="file"><did><unittitle>Rational approximation for non-linear ordinary differential equations</unittitle><container id="aspace_690771ee9bb5c7741189191a3ac99aa3" label="box [RS00777714]" type="box">31</container></did></c><c id="aspace_7e8562f61865320c6dbf3e5b7a54fc45" level="file"><did><unittitle>"N/D"—rational approximation</unittitle><container id="aspace_c33631ad74be642e0fc12d506f1f739d" label="box [RS00777714]" type="box">31</container></did></c><c id="aspace_33e77c83e59ab94ee0f7ffc3a23b6da9" level="file"><did><unittitle>Discussion on the paper "Rational Approximations for a Hamiltonian System"</unittitle><container id="aspace_4254a29230794d23486ae305a6920394" label="box [RS00777714]" type="box">31</container></did></c><c id="aspace_15b840c5fce5f460898b8cb732694d28" level="file"><did><unittitle>Non-linear approximation: general discussions</unittitle><container id="aspace_d396b81bd5029d138a0bd3081a5dc4ba" label="box [RS00777714]" type="box">31</container></did></c><c id="aspace_5847a8d445403e0edae20f483aa5fe52" level="file"><did><unittitle>Non-linear approximation for ordinary differential equation</unittitle><container id="aspace_57a2fc9aeca8ed6270e8092795210a41" label="box [RS00777714]" type="box">31</container></did></c><c id="aspace_f3f16dcdd02c82a2ae4c66ffb07e1df0" level="file"><did><unittitle>Non-linear approximation for periodic orbits in a Hamiltonian System</unittitle><container id="aspace_6678a67ea4f21415e2e2e6af3c78e173" label="box [RS00777714]" type="box">31</container></did></c><c id="aspace_507e27526e69c886c329921eb461463a" level="file"><did><unittitle>Non-linear oscillations</unittitle><container id="aspace_15c45bf9f07345b5e663f75a6ebe6502" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_68bf37c17a61383c08fedf0fc19a02ee" level="file"><did><unittitle>Non-linear dynamics</unittitle><container id="aspace_9693612749f26ddfc379977b10f43a43" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_e09a29a0132aa64f958c552acceafac8" level="file"><did><unittitle>Singular point approximation—solution of D.E. at an assumed pole</unittitle><unitdate datechar="creation">[1980s?]</unitdate><container id="aspace_89981c3bf9d10f49e2f825ba35af1292" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_62317c1dcbe0ca95e6846dd72b712dd5" level="file"><did><unittitle>Singularities and bifurcation</unittitle><container id="aspace_31d6764f0dbe8c2d699dfc5464b4ce70" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_480a14d378f7b03e6979a70aa93de051" level="file"><did><unittitle>(Equation) periodic solutions</unittitle><container id="aspace_1be2297e1ca666dd5ffaba750108de9d" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_de1bf671636b99fbc6e4f1bb6ac98be6" level="file"><did><unittitle>Bifurcation and vanishing of Henyey matrix and other difference equations</unittitle><container id="aspace_c43b81c090296c99b2240743119e1c37" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_505d24b05467e303a13e2321e31e4ae2" level="file"><did><unittitle>"Implicit" form of solutions to ordinary difference equations</unittitle><container id="aspace_4084cbaf6aa5a9fea253221c0fdae733" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_774f744ebed46e135379a14ab5d8554d" level="file"><did><unittitle>Difference equations with noise</unittitle><container id="aspace_fb8fde7225ee2e07074dd9c13be03d5e" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_44727e3853233bf09e739a6cb519a841" level="file"><did><unittitle>Stretched coordinate systems</unittitle><container id="aspace_eaffb12d57b58cf2e177e4a65452ed31" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_a7c49a1a53fe34ae5214aeb4dc4b3e20" level="file"><did><unittitle>Miscellaneous</unittitle><container id="aspace_f03e48f7a2160c68db123adc97d6e3c9" label="box [RS00777722]" type="box">32</container></did></c><c id="aspace_72c8914ae47268e3b65edc1d19df72f6" level="file"><did><unittitle>Talk on Non-linear mechanics (Fourier-Pade), New York University</unittitle><container id="aspace_a028887c799ffffb5d29bf437005d60f" label="box [RS00777722]" type="box">32</container></did></c></c><c id="aspace_188959bd2c43b5eaaa5a1ef44aa1589a" level="series"><did><unittitle>Series IV: Numerical Hydrodynamics</unittitle></did><c id="aspace_e9b8dae5ed3a15bc6186d1a908188196" level="file"><did><unittitle>Numerical hydrodynamics: beam schemes</unittitle><container id="aspace_1cdd72786d4e63ae27cf59738e28cf4b" label="box [RS00777730]" type="box">33</container></did></c><c id="aspace_3504cf0cd7b2b1224e12b5b0c7f218a6" level="file"><did><unittitle>Beam scheme</unittitle><container id="aspace_51b2cb67dc243cd60835a0d291d560d9" label="box [RS00777730]" type="box">33</container></did></c><c id="aspace_34e83f16eb8a2aeb2a35d5787adaa2d6" level="file"><did><unittitle>Continuous beam scheme</unittitle><container id="aspace_5bdc87da745d8738aea872b620c69af6" label="box [RS00777730]" type="box">33</container></did></c><c id="aspace_becc2765ce8a6533f845df39f8f37866" level="file"><did><unittitle>Three-dimensional axisymmetric cylindrical beam scheme with body force</unittitle><container id="aspace_4a582dffef3c42d5dd8e3b1f70b6ee41" label="box [RS00777730]" type="box">33</container></did></c><c id="aspace_87186a6a7ed232f1d0e97da530349fb4" level="file"><did><unittitle>Numerical Hydrodyamics from gas-kinetic theory</unittitle><container id="aspace_0fbc9b6dab6c89b9db813c678a96a943" label="box [RS00777749]" type="box">34</container></did></c><c id="aspace_a5db04ab11d4a38a767a8254d10ba282" level="file"><did><unittitle>Numerical Navier-Stokes solution from gas-kinetic theory-K Xu, and K Prendergast</unittitle><container id="aspace_7d528bd3c93bf3f9c42c0c70506e89c6" label="box [RS00777749]" type="box">34</container></did></c><c id="aspace_01abd4022a4aff42b5fd8147d850888c" level="file"><did><unittitle>Numerical Navier-Stokes solution from gas-kinetic theory—Kun Xu and Kevin Prendergast</unittitle><container id="aspace_bb15028e1d9ea5574f8aed4f77143a2d" label="box [RS00777749]" type="box">34</container></did></c><c id="aspace_c5f6c50422986202ce732992ac0b69f9" level="file"><did><unittitle>Paper II: final copy</unittitle><container id="aspace_8b20e96e7ba744c40f3b4ca58f93ae56" label="box [RS00777749]" type="box">34</container></did></c><c id="aspace_24b94ec74ebe7d5423683a2aebc9df63" level="file"><did><unittitle>Paper II: KX and KHP Navier-Stokes Paper</unittitle><container id="aspace_bec29808306f64e8705b1be9cc0de953" label="box [RS00777749]" type="box">34</container></did></c><c id="aspace_e4880f78e485d5258a8c1390a12060fa" level="file"><did><unittitle>Applied Math Seminar Notes (non-linear equations)</unittitle><container id="aspace_8126c34ca7ec0d305250b5b6a1d658aa" label="box [RS00777749]" type="box">34</container></did></c><c id="aspace_404f24bd1a63d50253334488f79ccbb9" level="file"><did><unittitle>Numerical Hydro-Spare</unittitle><container id="aspace_a17055a5bc7dc7f96521b75bf5c915c8" label="box [RS00777757]" type="box">35</container></did></c><c id="aspace_8dc5b58ccecd926d4c2b176d9ce43a74" level="file"><did><unittitle>Miscellaneous notes on non-linear dynamics and hydrodynamics Codes</unittitle><container id="aspace_42534356fc5dc50fc0cdd3864eca5831" label="box [RS00777757]" type="box">35</container></did></c><c id="aspace_c9ec16fd603616c5a537b6e12b4a3db6" level="file"><did><unittitle>Difference scheme from Hamiltonian principle</unittitle><container id="aspace_c52cff45173f2cffcaa747e23717c89e" label="box [RS00777757]" type="box">35</container></did></c><c id="aspace_1f07a180591be4f2f3f2099d82ccdd2e" level="file"><did><unittitle>Talk given at Supercomputer Conference, Santa Clara</unittitle><unitdate datechar="creation">1989</unitdate><container id="aspace_a8bf6263c5a410e84c93b18a9c6f7540" label="box [RS00777757]" type="box">35</container></did></c><c id="aspace_aa5feebc9bfe5b66bfea4f914d996b5c" level="file"><did><unittitle>Numerical hydrodynamics—talks at, Woods Hole &amp; Columbia University</unittitle><unitdate datechar="creation">7/25/2000 &amp; 9/27/2000</unitdate><container id="aspace_819441fdeb2fe6c754f572a354a6d3cc" label="box [RS00777757]" type="box">35</container></did></c><c id="aspace_27be51ba811c85aa318d936302ba6957" level="file"><did><unittitle>Applied Math Seminar Notes (non-linear equations)</unittitle><container id="aspace_a180b7c44920c8a7c7ca7d3a4e002d9e" label="box [RS00777757]" type="box">35</container></did></c></c><c id="aspace_a83271e06e74b38e52e8912a07e893aa" level="series"><did><unittitle>Series V: Applications of Hydrodynamics and Rarified Gas Dynamics</unittitle></did><c id="aspace_4e24481d858fd8ec9cbc545383bd0ac7" level="file"><did><unittitle>Slider bearing (for IBM Research)</unittitle><unitdate datechar="creation">1980s</unitdate><container id="aspace_f22b55566a43a08e97847f4a2734a324" label="box [RS00777757]" type="box">35</container></did></c><c id="aspace_23f2b6d67ebcb76d2fa08de2dd021616" level="file"><did><unittitle>Long mean-free-path approximation for slider bearing</unittitle><unitdate datechar="creation">1980s</unitdate><container id="aspace_891b18c339ed1df045b04ea0a114784d" label="box [RS00777757]" type="box">35</container></did></c><c id="aspace_025ce9553ab1e19baf40280900ce8110" level="file"><did><unittitle>Viscous flow with surface tension (for IBM Research</unittitle><unitdate datechar="creation">[1980s?]</unitdate><container id="aspace_65d3fa73585e8972a0fb515f72f5856b" label="box [RS00777765]" type="box">36</container></did></c><c id="aspace_7cc2a6f9e413972e3b8f758ea83dd45b" level="file"><did><unittitle>Water waves (test cases) (for IBM Research)</unittitle><unitdate datechar="creation">1980</unitdate><container id="aspace_39d5508a403cd6ae24b848710209d116" label="box [RS00777765]" type="box">36</container></did></c></c><c id="aspace_18d98b12ee0ed4d379de923be818d950" level="series"><did><unittitle>Series VI: Miscellaneous</unittitle></did><c id="aspace_350037c8fcb1ee7932061ec185041a4e" level="file"><did><unittitle>Optics (and singularities)—Catastrophe Optics?</unittitle><unitdate datechar="creation">1980</unitdate><container id="aspace_187d7c1dce40690bd7fd7b584219a45b" label="box [RS00777765]" type="box">36</container></did></c><c id="aspace_26c0881c9880563a0329761c0207606e" level="file"><did><unittitle>Spectral Line Formation</unittitle><container id="aspace_21d5cfe09f93cfb905deb66d254e54af" label="box [RS00777765]" type="box">36</container></did></c><c id="aspace_095c46123bb2d2e9c083b9c322c53625" level="file"><did><unittitle>Photoelectrical Photometry</unittitle><container id="aspace_abbb7923c564906e876450203db2985d" label="box [RS00777765]" type="box">36</container></did></c><c id="aspace_ede6dd3bb54c633f2d5f2045b40b3208" level="file"><did><unittitle>Thomas-Fermi quantization</unittitle><container id="aspace_80e4ff253075afe4898680fc98462b5f" label="box [RS00777765]" type="box">36</container></did></c><c id="aspace_04d4531f040fc4b1c087f084749ead1e" level="file"><did><unittitle>Computation of curves of constant P (a,b,c)</unittitle><container id="aspace_98618bdfbb42104d11b7e896b412f8b3" label="box [RS00777765]" type="box">36</container></did></c><c id="aspace_b1ed131e7ff5ccd471c6ec8cc80c96e7" level="file"><did><unittitle>Statistics</unittitle><container id="aspace_af8588ab1f2ba1b843081224e78302b1" label="box [RS00777765]" type="box">36</container></did></c><c id="aspace_a22110e680c1cedce91ca50ad2966679" level="file"><did><unittitle>Research Proposals: National Science Foundation</unittitle><container id="aspace_1732fc9de7e4b7e04e69a3235ee5eaa6" label="box [RS00777765]" type="box">36</container></did></c></c><c id="aspace_59d786c15fa8d781a69f3212db0e1877" level="series"><did><unittitle>Series VII: Published Papers</unittitle></did><c id="aspace_3addc5aa01b10d99e41f0463d71809ff" level="file"><did><unittitle>KHP Bibliography</unittitle><container id="aspace_596b52545ec86a43454b834d71c9b109" label="box [RS00777773]" type="box">37</container></did></c><c id="aspace_aed45ba84de3d5c705a05860ab83d25c" level="file"><did><unittitle>Reprints of K Prendergast</unittitle><container id="aspace_e57542dc5af9db813f06b26903be1ebc" label="box [RS00777773]" type="box">37</container></did></c><c id="aspace_edd72602c618c8a0be1f57be3894d1a7" level="file"><did><unittitle>Marseille Collaboration Papers</unittitle><container id="aspace_65d3906350eb1faa0580d74ba76fbe2a" label="box [RS00777773]" type="box">37</container></did></c><c id="aspace_5f51135214816ee56e8beb204035ae77" level="file"><did><unittitle>Prendergast, Kevin On the color-magnitude diagram of the globular cluster Centauri</unittitle><unitdate datechar="creation">1954</unitdate><physdesc id="aspace_62874fcc0231081c2d8477b78cb50468">Ph.D. thesis</physdesc><container id="aspace_114a69187f24a7de5555c370b29d6065" label="box [RS00777773]" type="box">37</container></did></c><c id="aspace_7c8b5e393d1ed6d1b88fa8d34150b90d" level="file"><did><unittitle>Some published papers related to two-fluid model for stars and gas in galaxies</unittitle><container id="aspace_53f51aa05b40f0505b2e711b9f12699b" label="box [RS00777897]" type="box">38</container></did></c><c id="aspace_a64afd8913e0ff0aab08b8e1bb659f4c" level="file"><did><unittitle>Nature of some X-Ray sources</unittitle><unitdate datechar="creation">1968</unitdate><container id="aspace_e5cc96eae9ae342fee111655b6290fce" label="box [RS00777897]" type="box">38</container></did></c><c id="aspace_0032e74c0a94502c9fe212c10fe2580a" level="file"><did><unittitle>Some published papers of galactic dynamics</unittitle><container id="aspace_987f39d563f55cf4cdc11aaf02247946" label="box [RS00777897]" type="box">38</container></did></c><c id="aspace_5b22bdb7b460ba9566b4acabb43be05c" level="file"><did><unittitle>Preprints of various published papers by K. Prendergast</unittitle><container id="aspace_03a6eb7b98085de99ba1d0fff0396072" label="box [RS00777897]" type="box">38</container></did></c><c id="aspace_1319bff1b95ef30efd108f6a91235bb0" level="file"><did><unittitle>University of Paris symposium on numerical simulation of formation and evolution of elliptical galaxies</unittitle><container id="aspace_adefad05150f70de5d714c9dcf35a911" label="box [RS00777897]" type="box">38</container></did></c><c id="aspace_7af09248cb0901127c2d09e23f6ed606" level="file"><did><unittitle>Tsiang, Eugene Yu-Kong The accretion disk model of X-ray stars, Columbia University</unittitle><unitdate datechar="creation">1977</unitdate><physdesc id="aspace_04a68f558e3f9cd3b9a5b618926e3b15">Ph.D. thesis</physdesc><container id="aspace_69e96978f915a5bb6ef2cf83caec4c07" label="box [RS00777897]" type="box">38</container></did></c><c id="aspace_7afa4b018cd7f0743b487f1986b238fb" level="file"><did><unittitle>Numerical hydrodynamic solutions based on BGK</unittitle><container id="aspace_1ca551da2ab61f857607b0fe825b5cf5" label="box [RS00777897]" type="box">38</container></did></c><c id="aspace_6a38949ec9a2e79f1810d78270ca57c8" level="file"><did><unittitle>Xu, Kun Numerical hydrodynamics from gas-kinetic theory, Columbia University</unittitle><unitdate datechar="creation">[n.d.]</unitdate><physdesc id="aspace_0e551efca339aec22bdb9cfb0da97a08">Ph.D. thesis</physdesc><container id="aspace_28347a12abf101757d8f6ecc6fbe2c54" label="box [RS00777781]" type="box">39</container></did></c><c id="aspace_d56ac5a8afb851287611ad7a27d010e1" level="file"><did><unittitle>Gravitational potential of a disk spiral galaxy—B. Barbanis and K. Prendergast</unittitle><container id="aspace_1ac758b6bf600a933e366471a8572a55" label="box [RS00777781]" type="box">39</container></did></c><c id="aspace_e86fa604f78fae65bed071c92fcfd1c9" level="file"><did><unittitle>Time-Independent Gravitational Fields in the BGK Scheme for Hydrodynamics (Slyz, Prendergast)</unittitle><container id="aspace_0c141dac1171ef75c159aafa65a78cbe" label="box [RS00777781]" type="box">39</container></did></c></c><c id="aspace_1d2507fcb6c270a6b2473f001993c056" level="series"><did><unittitle>Series VIII: Lecture Notes</unittitle></did><c id="aspace_1bb07d817949106cc7673631414f43db" level="subseries"><did><unittitle>Subseries VIII.1: Graduate School Courses (developed by K. Prendergast)</unittitle></did><c id="aspace_0c5a3a599b5609373ed7a4f860711ba5" level="file"><did><unittitle>Mechanics (Vol I, II)</unittitle><container id="aspace_97b27cd3f2996ef6512633765ee8ff9a" label="box [RS00777781]" type="box">39</container></did></c><c id="aspace_6dde58a0e01f5d1b07649f0bef3cc7de" level="file"><did><unittitle>Classical mechanics</unittitle><container id="aspace_e8fde7cef3b56bf1cf1c20bfaabcc3f2" label="box [RS00777781]" type="box">39</container></did></c><c id="aspace_1ae6097eea7702f2d4f50edf95b650b7" level="file"><did><unittitle>Basic astronomical data</unittitle><container id="aspace_93e00650c288cc11759d461b64ab77c4" label="box [RS00777781]" type="box">39</container></did></c><c id="aspace_86ad7fcf68d0cfa4a61609165354e106" level="file"><did><unittitle>Contemporary Astrophysics</unittitle><container id="aspace_e9a282bd5840843d8eabb1147f7aaebc" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_4378f944b002fe2045c99098a00c9ae0" level="file"><did><unittitle>Astrophysics</unittitle><container id="aspace_bf0c07b035e7ebef1b5be85ed8b3d2da" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_1cd420db80872ece273484fb88f287d7" level="file"><did><unittitle>Astrophysics II</unittitle><container id="aspace_37f333e185da6cd1f6403e63c1f019ed" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_bb9d8b22f9d40f4f5fcccb85529f02d7" level="file"><did><unittitle>Special relativity</unittitle><container id="aspace_f9bdf57074518d9f1897c6052425ba26" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_a4cf6539ccd6a2522f152b9d7d14c592" level="file"><did><unittitle>Relativity, gravitation, and black holes</unittitle><container id="aspace_f6f303ad5c380daa59dd249c150d72d1" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_2536c5aaa8716564c665025e23595da0" level="file"><did><unittitle>Radiation transfer</unittitle><container id="aspace_34f7a59c3649c3550ac880f6f86f0806" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_9c5bea46ffab2cbad8ba4f44418c167d" level="file"><did><unittitle>Gas stream in close binary systems</unittitle><container id="aspace_2d1d6af136e1175069fc6b83d2875834" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_90232311c8fe997fda2e8fa7cb0029cf" level="file"><did><unittitle>Galactic dynamics</unittitle><container id="aspace_85ab88cee8dbd122cc857a14fac8000f" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_7f61f4b8cd62f9a22d1990b09fe651c0" level="file"><did><unittitle>Galactic accretion</unittitle><container id="aspace_c3779faff03b339dc13043801d221ce4" label="box [RS00777900]" type="box">40</container></did></c><c id="aspace_26cb2acb197df281e025ba20a03435e9" level="file"><did><unittitle>Introduction to Stellar Evolution</unittitle><container id="aspace_8c899862f4fc560f991db16238eff13c" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_e010ccc8a68698100f38fbe1f666ae46" level="file"><did><unittitle>Electromagnetic theory</unittitle><container id="aspace_3d32ec2c9cdddefaecc933c7ad0df2ce" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_946275d26ef4ceb27abb35a69b742401" level="file"><did><unittitle>Statistical Mechanics and Thermodynamics</unittitle><container id="aspace_cea1cb6363f40e7d8d07dae08c49414f" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_8edbaf9f4238016523960f70d36e8dfe" level="file"><did><unittitle>Statistical Mechanics</unittitle><container id="aspace_9e18a4336fce42008f564c4a89657d21" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_db91dc8cea942d4d7d57a6f3694ed314" level="file"><did><unittitle>Prendergast Lectures for Correction</unittitle><unitdate datechar="creation">Jan 10, 1969</unitdate><container id="aspace_20e7ab592547f37d631107d97fa2d85b" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_498c965b20d13d8f8b12d2f5e591bc41" level="file"><did><unittitle>Statistical Mechanics</unittitle><container id="aspace_47b97dc1d94483b23f856cc728f9dcc4" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_f874f9888a367164cd2aca61fc1dd45f" level="file"><did><unittitle>Continuum Physics</unittitle><unitdate datechar="creation">Fall 78</unitdate><container id="aspace_2560dbfcc430fd91816165c8db56abb6" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_b7115a132fec4fa4bed87dec44978024" level="file"><did><unittitle>Hydro Course notes</unittitle><container id="aspace_9ffa5a9355d55387bc26e8b0582240ba" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_3da1db7b583fe1da2058b4e2497b64f8" level="file"><did><unittitle>Classical Theory of Radiation I</unittitle><container id="aspace_c2ea5764c294a5db653dad76c0481506" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_3e4e19c66081dce0363980e94909c545" level="file"><did><unittitle>Classical Theory of Radiation II</unittitle><container id="aspace_5f62db5283f251b7b93406606f9f6d89" label="box [RS00777790]" type="box">41</container></did></c></c><c id="aspace_d20b78592fad6281ba147714213aa522" level="subseries"><did><unittitle>Subseries VIII.2: Lecture notes on undergraduate courses</unittitle></did><c id="aspace_3a0b6f2b1f225355a5128f46bc545c8f" level="file"><did><unittitle>Special relativity</unittitle><container id="aspace_2b05204a3f25841ec831bf3d9b933cb4" label="box [RS00777790]" type="box">41</container></did></c></c><c id="aspace_a1917e6a499f49b0aeba7266d1dd80a4" level="subseries"><did><unittitle>Subseries VIII.3: Lecture notes on graduate school courses (developed by others)</unittitle></did><c id="aspace_dc685f7f97dbdf4e25c04d7362541eba" level="file"><did><unittitle>Galactic dynamics (by L. Woltijer)</unittitle><container id="aspace_38848703cfc9c9dd85457ca8781a1c8c" label="box [RS00777790]" type="box">41</container></did></c><c id="aspace_1d081abbd214ba59db0747419699875c" level="file"><did><unittitle>Quantum Mechanics</unittitle><container id="aspace_d28e90ad2d8dc3cb7df0459d6f5df7e7" label="box [RS00777919]" type="box">42</container></did></c><c id="aspace_ad09f1b8493ee2c81445d58932734bf0" level="file"><did><unittitle>Electromagnetic theory</unittitle><container id="aspace_a6a0abba4ed45f8a2c9334bc7c3bc64a" label="box [RS00777919]" type="box">42</container></did></c><c id="aspace_b25ceb2095bb11ec2069513990e5eafe" level="file"><did><unittitle>Classical mechanics</unittitle><container id="aspace_4376f4425203152c51d3c0c831f1e18b" label="box [RS00777919]" type="box">42</container></did></c><c id="aspace_587b12cab95f58a4ebf2b829ac7d6e8b" level="file"><did><unittitle>GNRI—Generalized Newton-Raphson code for boundary value problem developed by Norman Baker</unittitle><container id="aspace_c3ef6d72b95c0ccfa418295a351a3629" label="box [RS00777919]" type="box">42</container></did></c></c></c><c id="aspace_17d1bf3462f288f93c68fb2c3940e16d" level="series"><did><unittitle>Series IX: Astronomy Department/Professional Organizations</unittitle></did><c id="aspace_26d739eb05ef4beb4cdcf2b4a9b1377a" level="file"><did><unittitle>Astronomy Department/Professional Organizations material</unittitle><container id="aspace_3f6f7c53183a4c6fd9547b622524fe74" label="box [RS00777803]" type="box">43</container></did></c></c><c id="aspace_8a35c483eedcd3bbdca8dd7012ab3a6f" level="series"><did><unittitle>Series X: Ephemera</unittitle></did><c id="aspace_9c1a803ca43bc2f7586f1f2096226b8a" level="file"><did><unittitle>Diskettes</unittitle><container id="aspace_b0a46cdf575a8f41f5da038ea8b74482" label="box [RS00777927]" type="box">44</container></did></c><c id="aspace_8c0dc720b79b6441f5714c6e046c1521" level="file"><did><unittitle>Glass Plates</unittitle><container id="aspace_74788659d44085e240f998dc10e911ec" label="box [RS00777927]" type="box">44</container></did></c><c id="aspace_93d012273a69d9f2ecd6fe0b3a1be95e" level="file"><did><unittitle>Reel</unittitle><container id="aspace_600d36d4de7a89a42a2b9291667cb545" label="box [RS00777927]" type="box">44</container></did></c></c><c id="aspace_e2160aa7b1f22087ae527f00b7ac3a35" level="series"><did><unittitle>Series XI: Papers by Others</unittitle></did><c id="aspace_417fac7b72f257f761ab3f65676802fc" level="file"><did><unittitle>Papers by others</unittitle><container id="aspace_ba1a791cced07f6ec5cda1b16411dca2" label="box [RS00777811]" type="box">45</container></did></c><c id="aspace_8b000ef1f99b23fd1e6b7d9f1bbb273d" level="file"><did><unittitle>Papers by others</unittitle><container id="aspace_1c401f93ca4d63a1f2b7424f49517eb3" label="box [RS00777935]" type="box">46</container></did></c></c><c id="aspace_635e58d22370d4be4e746d8c8f07fc40" level="series"><did><unittitle>Series XII: Printed Material</unittitle></did><c id="aspace_b2c93425e4d5ffc8a332126b6bc31ff2" level="file"><did><unittitle>Printed Material</unittitle><container id="aspace_348ca9cb94669fd2889587a227cad253" label="box [RS00777820]" type="box">47</container></did></c><c id="aspace_2e1a3bf99f2019c6accab0547e3e66fd" level="file"><did><unittitle>Printed Material</unittitle><container id="aspace_2686e49f59fd48549bdeecf19bb62214" label="box [RS00777943]" type="box">48</container></did></c></c></dsc>
</archdesc>
</ead>
