Multiband optical photometry and bolometric light curve of the Type Ia supernova 2004S

被引:7
作者
Misra, K
Kamble, AP
Bhattacharya, D
Sagar, R
机构
[1] Aryabhatta Res Inst Observ Sci, Naini Tal 263129, India
[2] Raman Res Inst, Bangalore 560080, Karnataka, India
关键词
supernovae : general; supernovae : individual : SN2004S;
D O I
10.1111/j.1365-2966.2005.09059.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present BVRCIC broad-band CCD photometry of the Type Ia supernova SN 2004S, which appeared in the galaxy MCG-05-16-021, obtained during 2004 February 12 to March 22. We present multiband and bolometric light curves constructed using our data as well as other available data. The time of the B-band maximum and the peak magnitudes in different bands are obtained using fits of light-curve and colour templates. We clearly see a strong shoulder in the RC band and a second maximum in the I-C band. SN 2004S closely resembles SN 1992al after maximum. From the peak bolometric luminosity, we estimate the ejected mass of Ni-56 to be 0.41 M-circle dot.
引用
收藏
页码:662 / 668
页数:7
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