Luminosity of Evolving Supernova Remnants

Luminosity of Evolving Supernova Remnants

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.

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Veröffentlicht in:International Astronomical Union Colloquium 1988, Vol.101, p.435-438
Hauptverfasser: Cioffi, D.F., McKee, C.F.
Format: Artikel
Sprache:eng
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Zusammenfassung: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.
ISSN:0252-9211
DOI:10.1017/S0252921100102799