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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/591
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dc.contributor.authorZafarullah, S. N-
dc.contributor.authorNarasimhan, K. S. V. S-
dc.contributor.authorSastry, K. S-
dc.date.accessioned2005-12-05T09:09:06Z-
dc.date.available2005-12-05T09:09:06Z-
dc.date.issued1983-06-
dc.identifier.citationBASI, Vol. 11, No. 2, pp. 145-151en
dc.identifier.urihttp://hdl.handle.net/2248/591-
dc.description.abstractExpressions for the stellar velocity perturbations in colliding galaxies, valid for any distance of closest approach, are derived analytically under the impulsive approximation for spherical galaxies using a Newtonian potential with a softening parameter. The results are compared with those of earlier workers.en
dc.format.extent381411 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectGalaxiesen
dc.subjectCollisionsen
dc.subjectStellar Dynamicsen
dc.titleStellar velocity perturbations in colliding galaxies Ien
dc.typeArticleen
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