Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-19T03:44:04.407Z Has data issue: false hasContentIssue false
  • English
  • Français

X-ray Emission from Supernova Remnants in a Cloudy Medium

Published online by Cambridge University Press:  04 August 2017

Christopher F. McKee
Christopher F. McKee*
Affiliation:
Departments of Physics and Astronomy, University of California, Berkeley, CA 94720

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.

Young SNRs expand to much larger radii in a cloudy ISM than in a homogeneous medium, and they can have large variations in the pressure. The collision between supernova ejecta and an ambient cloud can result in an expanding high pressure region (a “secondary blast wave”). Observations of MSH 15–52 can be accounted for in this manner. X-ray emission from both young and older SNRs can provide an important probe for inferring the structure of the ISM.

Type
I. Young Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 87 - 97
Copyright
Copyright © Reidel 1983 

References

Ardavan, H.: 1973, Ap.J. 184, p. 435.CrossRefGoogle Scholar
Balbus, S.A., and McKee, C.F.: 1982, Ap.J. 252, p. 529.Google Scholar
Begelman, M., Sarazin, C., Hatchett, S., McKee, C., and Arons, J.: 1980, Ap.J. 238, p. 722.CrossRefGoogle Scholar
Blair, W.P., Kirshner, R.P., and Chevalier, R.A.: 1981, Ap.J. 247, p. 879.CrossRefGoogle Scholar
Blandford, R., Kennel, C., McKee, C.F., and Ostriker, J.P.: 1982, Nature (in press).Google Scholar
Bruhweiler, F.C., Gull, T.R., Kafatos, M., and Sofia, S.: 1980, Ap.J. (Letters) 238, p. L27.CrossRefGoogle Scholar
Castor, J., McCray, R., and Weaver, R.: 1975, Ap.J. (Letters) 200, p. L107.CrossRefGoogle Scholar
Chevalier, R.A.: 1975, Ap.J. 200, p. 698.Google Scholar
Chevalier, R.A.: 1976, Ap.J. 207, p. 872.CrossRefGoogle Scholar
Chevalier, R.A.: 1982, Ap.J. 258, p. 790.CrossRefGoogle Scholar
Chu, Y.H.: 1981, , .Google Scholar
Clarke, J.N.: 1976, M.N.R.A.S. 174, p. 393.Google Scholar
Cox, D.P.: 1979, Ap.J. 234, 863.Google Scholar
Cox, D.P., and Smith, B.W.: 1974, Ap.J. (Letters) 189, p. L105.Google Scholar
Cowie, L.L.: 1975, M.N.R.A.S. 173, p. 429.Google Scholar
Cowie, L.L., and McKee, C.F.: 1977, Ap.J. 211, p. 135.Google Scholar
Cowie, L.L., McKee, C.F., and Ostriker, J.P.: 1981, Ap.J. 247, p. 908.CrossRefGoogle Scholar
Dopita, M.A.: 1979, Ap.J. Suppl. 40, p. 455.CrossRefGoogle Scholar
Falk, S.W., and Arnett, W.D.: 1973, Ap.J. (Letters) 180, p. L65.Google Scholar
Field, G.B., Goldsmith, D.W., and Habing, H.J.: 1969, Ap.J. (Letters) 155, p. L149.CrossRefGoogle Scholar
Gull, S.F.: 1973, M.N.R.A.S. 161, p. 47.Google Scholar
Gull, S.F.: 1975, M.N.R.A.S. 171, p. 263.Google Scholar
Hamilton, A., Sarazin, C., and Chevalier, R.: 1982, Ap.J. (in press).Google Scholar
Hollenbach, D., and McKee, C.F.: 1979, Ap.J. Suppl. 41, p. 555.CrossRefGoogle Scholar
Kahn, F.D.: 1974, in “The Interstellar Medium,” ed. Pinkau, K. (Dordrecht:Reidel), p. 235.CrossRefGoogle Scholar
Long, K., Dopita, M., and Tuohy, I.: 1982, Ap.J. 260, p. 202.CrossRefGoogle Scholar
Mathewson, D.S.: 1983, this volume, p. 553.Google Scholar
McKee, C.F.: 1974, Ap.J. 188, p. 335.CrossRefGoogle Scholar
McKee, C.F.: 1982, in “Supernovae: A Survey of Current Research,” Rees, M. and Stoneham, R., eds. (Dordrecht: Reidel), p. 433.CrossRefGoogle Scholar
McKee, C.F., and Ostriker, J.P.: 1977, Ap.J. 218, p. 148.Google Scholar
Mills, B.Y.: 1983, this volume, p. 563.Google Scholar
Nulsen, P.E.J.: 1982, M.N.R.A.S. 198, p. 1007.Google Scholar
Peimbert, M., and van den Bergh, S.: 1971, Ap.J. 167, p. 223.CrossRefGoogle Scholar
Seward, F.D., and Harnden, F.R.: 1982, Ap.J. (Letters) 256, p. L45.Google Scholar
Seward, F.D., Harnden, F.R., Murdin, P., and Clark, D.H.: 1983, Ap.J. (in press).Google Scholar