SN 2002ap, the Hypernova of Class Ic

dc.contributor.author	Pandey, S. B
dc.contributor.author	Sahu, D. K
dc.contributor.author	Anupama, G. C
dc.contributor.author	Bhattacharya, D
dc.contributor.author	Sagar, R
dc.date.accessioned	2008-06-06T07:52:07Z
dc.date.available	2008-06-06T07:52:07Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 351 - 352	en
dc.identifier.uri	http://hdl.handle.net/2248/2416
dc.description.abstract	The 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.extent	62870 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/2003BASI...31..351P	en
dc.subject	Photometry	en
dc.subject	Hypernovae	en
dc.subject	Light-curve	en
dc.title	SN 2002ap, the Hypernova of Class Ic	en
dc.type	Article	en