Photometric study of type Ia supernova SN 2002hu

Sahu, D. K. ; Anupama, G. C. ; Prabhu, T. P. (2006) Photometric study of type Ia supernova SN 2002hu Monthly Notices of the Royal Astronomical Society, 366 (2). pp. 682-688. ISSN 0035-8711

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Official URL: http://mnras.oxfordjournals.org/content/366/2/682....

Related URL: http://dx.doi.org/10.1111/j.1365-2966.2005.09893.x

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.

Item Type:Article
Source:Copyright of this article belongs to Oxford University Press.
Keywords:Supernovae: General; Supernovae: Individual: SN 2002hu; Galaxies: Individual: MCG+6−6−12
ID Code:100745
Deposited On:10 Dec 2016 12:42
Last Modified:10 Dec 2016 12:42

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