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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1867
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dc.contributor.authorNarasimhan, K. S. V. S-
dc.contributor.authorSastry, K. S-
dc.contributor.authorAlladin, S. M-
dc.date.accessioned2007-10-09T10:56:16Z-
dc.date.available2007-10-09T10:56:16Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol. 24, No. 4, pp. 805 - 811en
dc.identifier.urihttp://hdl.handle.net/2248/1867-
dc.description.abstractwe propose a classification scheme for colliding galaxies based on the fractional changes in their binding energy and the orbital energy. We give examples of actual observed pairs of interacting galaxies for the various types of collisions proposed in the scheme.en
dc.format.extent463755 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..805Nen
dc.subjectGalaxiesen
dc.subjectCollidingen
dc.titleClassification of colliding galaxiesen
dc.typeArticleen
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