Abstract
Among the mechanisms of X-ray emissions from supernovae, we focus on the circumstellar interaction. In particular, we relate the new X-ray features of SN1993J to the hydrodynamical instabilities in the ejecta. First, we model the early-time two component spectral feature by invoking instabilities in the dense cooling shell in the ejecta. Second, we model the gradual increase in the X-ray light curve as X-rays emitted from the reverse shocked ejecta; here the model requires a large scale change in the density distribution due to Rayleigh-Taylor instabilities around the core-envelope interface.
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© 1998 Springer Science+Business Media Dordrecht
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Nomoto, K., Suzuki, T. (1998). X-Rays from Supernova 1993J and Ejecta Instabilities. In: Koyama, K., Kitamoto, S., Itoh, M. (eds) The Hot Universe. International Astronomical Union / Union Astronomique Internationale, vol 188. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4970-9_6
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DOI: https://doi.org/10.1007/978-94-011-4970-9_6
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-5059-0
Online ISBN: 978-94-011-4970-9
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