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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2126
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dc.contributor.authorDewangan, G. C-
dc.contributor.authorSingh, K. P-
dc.contributor.authorBhat, P. N-
dc.date.accessioned2008-03-05T11:21:48Z-
dc.date.available2008-03-05T11:21:48Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 375 - 376en
dc.identifier.urihttp://hdl.handle.net/2248/2126-
dc.description.abstractBased on VBT observations, we report multicolour broadband study of a lenticular galaxy, NGC 4753 with prominent dust lanes. The extinction curve derived for NGC 4753 is similar to the Galactic extinction curve. The dust mass estimated from optical extinction is 1.51 x 105 M? and from the far infrared fluxes observed with Infrared Astronomical Satellite (IRAS) is 3.46 x 105 M?. The dust observed within NGC 4753 can be argued to be internal in origin.en
dc.format.extent207570 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..375Den
dc.subjectGalaxiesen
dc.subjectDust extinctionen
dc.subjectFIRen
dc.titleMulticolour broadband study of a lenticular galaxy : NGC 4753en
dc.typeArticleen
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