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The stability of a model galaxy.

dc.contributor.advisorAlar Toomre.en_US
dc.contributor.authorZang, Thomas Arthuren_US
dc.date.accessioned2008-10-02T19:14:02Z
dc.date.available2008-10-02T19:14:02Z
dc.date.issued1976en_US
dc.identifier.urihttp://dspace.mit.edu/handle/1721.1/27444en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/27444
dc.descriptionThesis. 1976. Ph.D.--Massachusetts Institute of Technology. Dept. of Mathematics.en_US
dc.descriptionMicrofiche copy available in Archives and Science.en_US
dc.descriptionBibliography: leaves 203-204.en_US
dc.format.extent204 leavesen_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/27444en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectMathematicsen_US
dc.subject.lcshGalaxiesen_US
dc.subject.lcshDisks, Rotatingen_US
dc.subject.lcshStabilityen_US
dc.subject.lcshCelestial mechanicsen_US
dc.titleThe stability of a model galaxy.en_US
dc.typeThesisen_US
dc.description.degreePh.D.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Mathematics
dc.identifier.oclc02404125en_US


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