Modeling the Radio and X-ray Emission of SN 1993J and SN 2002ap

Details Modeling the Radio and X-ray Emission of SN 1993J and SN 2002ap Modeling the Radio and X-ray Emission of SN 1993J and SN 2002ap

2004-04-14

arxiv.org/abs/astro-ph/0404267v1

Astronomy and Astrophysics

Astrophysics

10 pages, 2 figures. Uses svmult.cls. To appear in proceedings of IAU Colloquium 192 "Supernovae (10 years of SN 1993J)", Apri

Scientific paper

Modeling of radio and X-ray observations of supernovae interacting with their circumstellar media are discussed, with special application to SN 1993J and SN 2002ap. We emphasize the importance of including all relevant physical mechanisms, especially for the modeling of the radio light curves. The different conclusions for the absorption mechanism (free-free or synchrotron self-absorption), as well as departures from an $\rho \propto r^{-2}$ CSM, as inferred by some authors, are discussed in detail. We conclude that the evidence for a variation in the mass loss rate with time is very weak. The results regarding the efficiencies of magnetic field generation and relativistic particle acceleration are summarized.

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