Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1554
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dc.contributor.authorSridhar, S.-
dc.date.accessioned2006-11-30T11:14:46Z-
dc.date.available2006-11-30T11:14:46Z-
dc.date.issued1989-06-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1989, Vol.238, p1159-1163en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/1554-
dc.descriptionOpen Accessen
dc.description.abstractThe Lewis (1968) invariant of the time-dependent harmonic oscillator is used to construct exact time-dependent, uniform density solutions of the collisionless Boltzmann equation. The spatially bound solutions are time-periodic.en
dc.format.extent8338 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishing for the Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query? 1989MNRAS.238.1159Sen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989MNRAS.238.1159S&link_type=ARTICLE&db_key=ASTen
dc.rights(1989) Royal Astronomical Societyen
dc.subjectCOMPUTATIONAL ASTROPHYSICS,en
dc.subjectSTELLAR OSCILLATIONS,en
dc.subjectSTELLAR SYSTEMS,en
dc.subjectBOLTZMANN TRANSPORT EQUATION,en
dc.subjectEQUATIONS OF MOTIONen
dc.titleUndamped oscillations of homogenous collisionless stellar systemsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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