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Luminosity of Evolving Supernova Remnants
Published online by Cambridge University Press: 12 April 2016
Abstract
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
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