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- W1580905829 abstract "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." @default.
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- W1580905829 date "2005-11-21" @default.
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- W1580905829 title "Modeling the Radio and X-ray Emission of SN 1993J and SN 2002ap" @default.
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- W1580905829 doi "https://doi.org/10.1007/3-540-26633-x_8" @default.
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