Photometric study of type Ia supernova SN 2002hu

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1654

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DC Field	Value	Language
dc.contributor.author	Sahu, D. K	-
dc.contributor.author	Anupama, G. C	-
dc.contributor.author	Prabhu, T. P	-
dc.date.accessioned	2007-06-18T05:19:14Z	-
dc.date.available	2007-06-18T05:19:14Z	-
dc.date.issued	2006-01	-
dc.identifier.citation	MNRAS, Vol. 366, No. 2, pp. 682–688	en
dc.identifier.uri	http://hdl.handle.net/2248/1654	-
dc.description	Restricted Access	en
dc.description.abstract	Optical UBVRI photometry of the type Ia supernova (SN Ia) SN 2002hu covering the period from −2 to +73 d since B maximum is presented. The supernova reached at maximum brightness in B on JD 245 2591.78 ± 0.5 with an apparent magnitude of 16.83 ± 0.02 mag and a relatively blue colour (B−V) =−0.08 ± 0.04 mag. The luminosity decline rate of Δm15(B) = 1.00 ± 0.05 indicates an absolute B magnitude at maximum of MmaxB=−19.38 ± 0.3. The estimated absolute B magnitude, together with the photometric evolution, indicate SN 2002hu was slightly overluminous compared to the average SNe Ia. The distance modulus to the parent galaxy is estimated to be μ= 36.04 ± 0.20.	en
dc.format.extent	667245 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Blackwell Publishing	en
dc.relation.uri	http://www.blackwell-synergy.com/doi/abs/10.1111/j.1365-2966.2005.09893.x	en
dc.subject	Supernovae: general	en
dc.subject	Galaxies: individual	en
dc.title	Photometric study of type Ia supernova SN 2002hu	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Publications based on data from IAO, Hanle

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