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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/666
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dc.contributor.authorNarasimhan, K. S. V. S-
dc.contributor.authorAlladin, S. M-
dc.date.accessioned2005-12-08T05:01:29Z-
dc.date.available2005-12-08T05:01:29Z-
dc.date.issued1985-12-
dc.identifier.citationBASI, Vol. 13, No. 4, pp. 359-362en
dc.identifier.urihttp://hdl.handle.net/2248/666-
dc.description.abstractLimber`s (1965) tidal model for the interacting pair of galaxies VV 117 ( = Arp 143 = NGC 2444-45) is improved upon in the light of subsequent H I observations. It is proposed that the spiral Sc component is being disrupted by the tidal effects of the elliptical (which is about twice as massive) in a close collision in a bound orbit.en
dc.format.extent332627 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectInteracting Galaxiesen
dc.subjectStellar dynamicsen
dc.titleA Tidal model for the inetracting pair of galaxies VV 117en
dc.typeArticleen
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