Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2416
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dc.contributor.authorPandey, S. B-
dc.contributor.authorSahu, D. K-
dc.contributor.authorAnupama, G. C-
dc.contributor.authorBhattacharya, D-
dc.contributor.authorSagar, R-
dc.date.accessioned2008-06-06T07:52:07Z-
dc.date.available2008-06-06T07:52:07Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 351 - 352en
dc.identifier.urihttp://hdl.handle.net/2248/2416-
dc.description.abstractThe supernova SN 2002ap was discovered in the outer regions of the nearby spiral M74 on January 29.4 UT. Early photometric and spectroscopic observations indicate the supernova belongs to the class of Ic hypernova. Late time (After JD 2452500) light curve decay slopes are similar to that of the hypernovae SN 1997ef and SN 1998bw. We present here the BVRI photometric light curves and colour evolutions of SN 2002ap to investigate the late time nature of the light curve.en
dc.format.extent62870 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..351Pen
dc.subjectPhotometryen
dc.subjectHypernovaeen
dc.subjectLight-curveen
dc.titleSN 2002ap, the Hypernova of Class Icen
dc.typeArticleen
Appears in Collections:BASI Publications
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