Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-12T15:29:47.671Z Has data issue: false hasContentIssue false

The Evolution of Older Remnants

Published online by Cambridge University Press:  12 April 2016

S.A.E.G. Fall*
Affiliation:
Department of Applied Mathematical Studies, The University, Leeds LS2 9JT, U.K

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.

An older remnant will be defined as one in which radiative cooling occurs somewhere and has swept up enough mass for the details of the explosion to be less important than the state of the interstellar medium in which the explosion occurred. Without discussing any particular remnant in detail, I will consider how large and small scale density variations in the ambient medium affect the appearance and energetics of such remnants. Finally I will show that radiative instabilities can modify the emission spectrum of radiative shocks in such a way that a naive interpretation of these spectra can be very misleading.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1988

References

Avedisova, V.S. 1974. Sov. Astron., 18, 283.Google Scholar
Bertschinger, E. 1986. Astrophys. J., 304, 154.CrossRefGoogle Scholar
Bryson, A.E. & Gross, R.W.F. 1961. J. Fluid Mech., 10, 1.Google Scholar
Charles, P.A, Kahn, S.M. & McKee, C.F. 1985. Astrophys. J., 295, 456.CrossRefGoogle Scholar
Chevalier, R.A. & Gardner, J. 1974. Astrophys. J., 192, 457.CrossRefGoogle Scholar
Chevalier, R.A. & Imamura, J.N. 1982. Astrophys. J., 261, 543.Google Scholar
Chevalier, R.A. & Theys, J.C. 1975. Astrophys. J., 195, 53.CrossRefGoogle Scholar
Cox, D.P. 1972. Astrophys. J., 178, 159.CrossRefGoogle Scholar
Falle, S.A.E.G. 1975. Mon. Not. R. astr. Soc., 172, 55.Google Scholar
Falle, S.A.E.G. 1981. Mon. Not. R. astr. Soc., 195, 1011.Google Scholar
Falle, S.A.E.G. & Garlick, A.R. 1982. Mon. Not. R. astr. Soc., 201, 635.CrossRefGoogle Scholar
Falle, S.A.E.G., Garlick, A.R. & Pidsley, P.H. 1984. Mon. Not. R. astr. Soc., 208, 925.Google Scholar
Fesen, R.A., Blair, W.P. & Kirshner, R.P. 1982. Astrophys. J., 262, 171.Google Scholar
Garlick, A.R. 1983. J. Comput. Phys., 52, 427.Google Scholar
Guli, S.F. 1973. Mon. Not. R. astr. Soc., 161, 47.Google Scholar
Hamilton, A.J.S. 1985. Astrophys. J., 291, 523.Google Scholar
Heathcote, S.R. & Brand, P.W.J.L. 1983. Mon. Not. R. astr. Soc., 203, 67.CrossRefGoogle Scholar
Imamura, J.N., Wolff, M.T.. & Durisen, R.H. 1984. Astrophys. J., 276, 667.Google Scholar
Innes, D.E., Giddings, J.R. & Falle, S.A.E.G. 1987. Mon. Not. R. astr. Soc., 226, 67.Google Scholar
Kahn, F.D. 1976. Astr. & Astrophys., 50, 145.Google Scholar
Langer, S.H., Chanmugam, G. & Shaviv, G. 1981. Astrophys. J., 245, L23.Google Scholar
Langer, S.H., Chanmugam, G. & Shaviv, G. 1982. Astrophys. J., 258, 289.CrossRefGoogle Scholar
Laumbach, D.D. & Probstein, R.F. 1969. J. Fluid Mech., 54, 229.Google Scholar
McCray, R., Stein, R.F. & Kafatos, M. 1975. Astrophys. J., 196, 565.Google Scholar
McKee, C.F. & Cowie, L.L. 1975. Astrophys. J., 195, 715.Google Scholar
Nittmann, J., Falle, S.A.E.G. & Gaskell, P.H. 1982. Mon. Not. R. astr. Soc., 201, 833.Google Scholar
Raymond, J.C., Black, J.H., Dupree, A.K. & Hartmann, L. 1980. Astrophys. J., 238, 881.CrossRefGoogle Scholar
Sgro, A.G. 1975. Astrophys. J., 197, 621. Google Scholar
Shull, P., Dyson, J.E., Kahn, F.D. & West, K.A. 1985. Mon. Not. R. astr. Soc. 212, 799.CrossRefGoogle Scholar
Tenorio-Tagle, G. & Rozyczka, M. 1984. Astr. & Astrophys., 137, 276.Google Scholar
Tenorio-Tagle, G., Rozyczka, M. & Yorke, H.W. 1985. Astron. & Astrophys., 148, 52.Google Scholar
Tomisaka, K. & Ikeuchi, S. 1986. Publ. Astron. Soc. Japan,, 38, 697.Google Scholar
van Dyke, M. 1982. An Album of Fluid Motion, Parabolic Press.Google Scholar
Whitham, G.B. 1974. Linear and Nonlinear Waves, Wiley Interscience, chapter 8.Google Scholar
Woltjer, L. 1972. Ann. Rev. Astron. Astrophys., 10, 129.Google Scholar
Woodward, P.R. 1976. Astrophys. J., 207, 484.Google Scholar