Tidal interactions in spherical galaxies

dc.contributor.author	Namboodiri, P. M. S
dc.date.accessioned	2008-03-15T11:15:51Z
dc.date.available	2008-03-15T11:15:51Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 2, pp. 397 - 399	en
dc.identifier.uri	http://hdl.handle.net/2248/2160
dc.description.abstract	Numerical simulations of equal mass galaxies, moving initially on a parabolic orbit, have been performed to see how the total energy of the system changes in close and wide encounters. The results are compared with those obtained using impulse approximation.	en
dc.format.extent	146395 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000BASI...28..397N	en
dc.subject	Galaxies	en
dc.subject	Interactions	en
dc.subject	Numerical simulations	en
dc.title	Tidal interactions in spherical galaxies	en
dc.type	Article	en