dc.contributor.author |
Arora, S |
|
dc.contributor.author |
Sahu, D. K |
|
dc.contributor.author |
Anupama, G. C |
|
dc.date.accessioned |
2012-06-11T13:51:36Z |
|
dc.date.available |
2012-06-11T13:51:36Z |
|
dc.date.issued |
2011-12 |
|
dc.identifier.citation |
ASP Conference Series, Vol. 451, pp. 275-278 |
en |
dc.identifier.isbn |
978-1-58381-784-1 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/5778 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
We present BVRI photometry and medium resolution spectroscopy of the supernova SN2007rw during ˜ 1 week to ˜ 7 months after discovery. This supernova was classified as a type IIb event, however, based on our analysis we suggest that SN 2007rw is a type IIL supernova. With an absolute B magnitude of M/sub B/= -18.5 magnitude at peak, it is a bright IIL event. The early spectrum of SN 2007rw shows H alpha and H Beta with weak P-Cygni absorption. The mass of /sup56/Ni synthesized in the explosion is estimated as ˜ 0.43 M/sub sun/. The metallicity of the host galaxy in the supernova region is found to be marginally subsolar. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of the Pacific |
en |
dc.relation.uri |
http://www.aspbooks.org/a/volumes/article_details/?paper_id=33727 |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2011ASPC..451..275A |
en |
dc.rights |
© Astronomical Society of the Pacific |
en |
dc.subject |
SN2007rw |
en |
dc.subject |
IIL Supernova |
en |
dc.title |
SN2007rw- A Type IIL Supernova |
en |
dc.type |
Article |
en |