Rapidly Interpreting UV-optical Light Curve Properties Using a “Simple” Modeling Approach
Core-collapse supernovae (CCSNe) have very distinct observational properties that depend on the composition of the progenitor star, the dynamics of the explosion mechanism, and the surrounding stellar wind environment. In recent years, due to the uncertainty behind the type of massive star that evol...
| Main Authors: | , , |
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| Language: | en |
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IOP PUBLISHING LTD
2017
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| Subjects: | |
| Online Access: | http://hdl.handle.net/10150/627104 http://arizona.openrepository.com/arizona/handle/10150/627104 |