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Luminosity of Evolving Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

D.F. Cioffi  and
C.F. McKee
D.F. Cioffi
Affiliation:
University of California, Berkeley, California, U.S.A
C.F. McKee
Affiliation:
University of California, Berkeley, California, U.S.A

Abstract

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We present an analytic kinematic model for the evolution of a supernova remnant beginning with the Sedov-Taylor adiabatic stage and continuing through the radiative stage. Using this model, we obtain the luminosity of the radiative shock and the hot interior.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 435 - 438
Copyright
Copyright © Cambridge University Press 1988

References

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