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Cosmic Explosions pp 59–69Cite as

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

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Part of the book series: Springer Proceedings in Physics ((SPPHY,volume 99))

Summary

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 ρ ∝ 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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Author information

Authors and Affiliations

  1. Department of Astronomy, Stockholm University, AlbaNova, 106 91, Stockholm, Sweden

    Claes Fransson & Claes-Ingvar Björnsson

Authors
  1. Claes Fransson
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  2. Claes-Ingvar Björnsson
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Editor information

Editors and Affiliations

  1. Depto. Astronomia y Astrofisica, Universidad de Valencia, Calle Dr. Moliner 50, 46100, Burjassot, Spain

    Juan-María Marcaide

  2. Naval Research Laboratory, Code 7213, Washington, DC, 20375-5320, USA

    Kurt W. Weiler

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Fransson, C., Björnsson, CI. (2005). Modeling the Radio and X-ray Emission of SN 1993J and SN 2002ap. In: Marcaide, JM., Weiler, K.W. (eds) Cosmic Explosions. Springer Proceedings in Physics, vol 99. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-26633-X_8

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