SN 2002ap, the hypernova of class Ic

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DC Field	Value	Language
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	2006-06-12T10:16:52Z	-
dc.date.available	2006-06-12T10:16:52Z	-
dc.date.issued	2003	-
dc.identifier.citation	Bulletin of the Astronomical Society of India, 2003, Vol.31, p351-352	en
dc.identifier.issn	0304-9523	-
dc.identifier.uri	http://hdl.handle.net/2289/1353	-
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	94876 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?2003BASI...31..351P	en
dc.rights	(2003) by the Astronomical Society of India.	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
Appears in Collections:	Research Papers (A&A)

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