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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2299
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dc.contributor.authorDas, M-
dc.contributor.authorChakraborty, D. K-
dc.date.accessioned2008-05-13T12:04:26Z-
dc.date.available2008-05-13T12:04:26Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 439 - 442en
dc.identifier.urihttp://hdl.handle.net/2248/2299-
dc.description.abstractTriaxial 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.extent230146 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..439Den
dc.subjectTriaxialen
dc.subjectHubble massen
dc.titleA family of triaxial mass models : Analytical study of its projected propertiesen
dc.typeArticleen
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