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X-ray emission from Reverse-Shocked Ejecta in Supernova Remnants
Published online by Cambridge University Press: 12 April 2016
Abstract
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.
- Type
- 4. Supernova Remnants, Soft X-ray Background
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- Copyright © Cambridge University Press 1990