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X-ray emission from Reverse-Shocked Ejecta in Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

Denis F. Cioffi and
Christopher F. McKee
Denis F. Cioffi
Affiliation:
NASA/Goddard Space Flight Center, Greenbelt, Maryland, U.S.A.
Christopher F. McKee
Affiliation:
University of California, Berkeley, California, U.S.A.

Abstract

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A simple physical model of the dynamics of a young supernova remnant is used to derive a straightforward kinematical description of the reverse shock. With suitable approximations, formulae can then be developed to give the X-ray emission of the reverse-shocked ejecta. The results are found to agree favorably with observations of SN1006.

Information

Type
4. Supernova Remnants, Soft X-ray Background
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990, pp. 164 - 167
Copyright
Copyright © Cambridge University Press 1990

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