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24 April 2024
 
  » arxiv » 0902.4059

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Radio Supernovae: Circum-Stellar Investigation (C.S.I.) of Supernova Progenitor Stars
Christopher J. Stockdale ; Kurt W. Weiler ; Nino Panagia ; Richard A. Sramek ; Schuyler D. Van Dyk ; Stefan Immler ; Dave Pooley ; J. M. Marcaide ; S. Ryder ; Matthew T. Kelley ; Christopher L. Williams ;
Date 24 Feb 2009
AbstractPrior to explosion, a supernova progenitor slowly loses significant amounts of its hydrogen envelope in a stellar wind. After the explosion, the blastwave interacts with this wind producing synchrotron emission. A year of radio observations allows us to probe the progenitor evolution for a thousand years. The EVLA and SKA would represent more than an order of magnitude improvement in our ability to explore the pre-explosion lives of a significantly large population of supernova progenitor stars. It will allow us to move beyond the crude optical classifications and develop a deeper physical understanding of how massive stars live and die.
Source arXiv, 0902.4059
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