A Tidal model for the inetracting pair of galaxies VV 117

dc.contributor.author	Narasimhan, K. S. V. S
dc.contributor.author	Alladin, S. M
dc.date.accessioned	2005-12-08T05:01:29Z
dc.date.available	2005-12-08T05:01:29Z
dc.date.issued	1985-12
dc.identifier.citation	BASI, Vol. 13, No. 4, pp. 359-362	en
dc.identifier.uri	http://hdl.handle.net/2248/666
dc.description.abstract	Limber`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.extent	332627 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Interacting Galaxies	en
dc.subject	Stellar dynamics	en
dc.title	A Tidal model for the inetracting pair of galaxies VV 117	en
dc.type	Article	en