NASA NTRS · 19910071679
X-ray emission from reverse-shocked ejecta in supernova remnants
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.
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Cioffi, Denis F., Mckee, Christopher F.. 1990-01-01. X-ray emission from reverse-shocked ejecta in supernova remnants. https://ntrs.nasa.gov/citations/19910071679
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