dc.contributor.author |
Chandra, P |
|
dc.contributor.author |
Ray, A |
|
dc.contributor.author |
Bhatnagar, S |
|
dc.date.accessioned |
2008-07-23T09:35:22Z |
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dc.date.available |
2008-07-23T09:35:22Z |
|
dc.date.issued |
2002-09 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 3, pp. 755 - 758 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2837 |
|
dc.description.abstract |
Multi-frequency observations of two radio bright SNe (SN1993J, SN1979C) carried out over a year with GMRT are presented. Their radio light curves trace the evolution of the mass loss in the stellar wind before the pre-supernova star exploded. Their spectra at low frequencies distinguish between the synchrotron self-absorption and free-free absorption based models. Two very similar type IIp SN1999gi and SN1999em were also observed and we comment on their progenitor mass. These observations of different subclasses of core-collapse supernovae will aid in defining their progenitors. |
en |
dc.format.extent |
126020 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
Core Collapse Supernovae |
en |
dc.subject |
SN1993J, SN 1979C-Progenitors |
en |
dc.title |
Radio Studies of young core collapse supernovae |
en |
dc.type |
Article |
en |