A family of triaxial mass models : Analytical study of its projected properties

dc.contributor.author	Das, M
dc.contributor.author	Chakraborty, D. K
dc.date.accessioned	2008-05-13T12:04:26Z
dc.date.available	2008-05-13T12:04:26Z
dc.date.issued	2001
dc.identifier.citation	BASI, Vol. 29, No. 3, pp. 439 - 442	en
dc.identifier.uri	http://hdl.handle.net/2248/2299
dc.description.abstract	Triaxial modified Hubble mass models are studied. The models are more general than those studied by earlier workers. The potential and the projected surface density of the mass models can be calculated analytically. The shapes of the isophotes and the profiles of ellipticity and position angles are studied. The inclusion of large number of terms in density function, allows one to produce a large variety of these profiles, which can be compared with observations.	en
dc.format.extent	230146 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/2001BASI...29..439D	en
dc.subject	Triaxial	en
dc.subject	Hubble mass	en
dc.title	A family of triaxial mass models : Analytical study of its projected properties	en
dc.type	Article	en