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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/319
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dc.contributor.authorSastry, Shankara. K-
dc.contributor.authorAlladin, S. M-
dc.date.accessioned2005-02-04T16:59:44Z-
dc.date.available2005-02-04T16:59:44Z-
dc.date.issued1981-09-
dc.identifier.citationBASI, Vol. 9, No. 3, pp. 249-254en
dc.identifier.urihttp://hdl.handle.net/2248/319-
dc.description.abstractThe dependence of the escape velocity of a pair of interacting identical spherical galaxies on their separation is studied using polyropic models for the galaxies. It is found that if the escape (parabolic) velocity of the pair is expressed in units of Vrms of the stars and the separation of the galaxies in units of mean radius of the galaxy, the relationship between these two quantities is independent of the mass distribution of the galaxies. This relationship is given.en
dc.format.extent301184 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectinteracting galaxiesen
dc.titleEscape velocities of interacting spherical galaxiesen
dc.typeArticleen
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