Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-12T15:47:54.009Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Cioffi, D.F., and McKee, C.F. 1987, Ap. J., in preparation (CM).Google Scholar
Cioffi, D.F., McKee, C.F., and Bertschinger, E. 1987, Ap. J., submitted (CMB).Google Scholar
Cox, D.P. 1986, Ap. J., 304, 771.Google Scholar
Dwek, E. 1981, Ap. J., 247, 614.Google Scholar
Graham, J.R., et al. 1987, Ap. J., 319, 126.Google Scholar
Kahn, F.D. 1976, Astr. Ap., 145, 50.Google Scholar
McKee, C.F. 1974, Ap. J., 188, 335.Google Scholar
McKee, C.F. and Ostriker, J.P. 1977, Ap. J., 218, 148.Google Scholar
Ostriker, J.P., and McKee, C.F. 1987, Rev. Mod. Phys, submitted.Google Scholar
Sedov, L.I. 1959, Similarity and Dimensional Methods in Mechanics, (New York: Academic Press).Google Scholar
Taylor, G.I. 1950, Proc. Royal Soc. London, 201A, 159.Google Scholar