Luminosity of Evolving Supernova Remnants
Abstract
The authors 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, they obtain the luminosity of the radiative shock and the hot interior.
- Publication:
-
IAU Colloq. 101: Supernova Remnants and the Interstellar Medium
- Pub Date:
- 1988
- Bibcode:
- 1988srim.conf..435C