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High Resolution Spectroscopy and Plasma Diagnostics of Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

Claude R. Canizares
Claude R. Canizares*
Affiliation:
Department of Physics and Center for Space ResearchMassachusetts Institute of Technology

Abstract

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The MIT group has used data from the Focal Plane Crystal Spectrometer on the Einstein Observatory to perform plasma diagnostics of four supernova remnants (SNRs), the Cygnus Loop, Puppis A, N132D, and Cas A. The ratio of luminosities of the forbidden line to resonance line of He-like ions of oxygen and neon allow us to show that all four SNRs depart from ionization equilibrium in that they are under-ionized for their electron temperatures. Thus despite the fact that their ages range from 300 yr to 20,000 yr, all four SNRs are still ionizing and, in that sense, are still young. We derive values of ionization time and electron temperature for one or more components in each remnant. The agreement between these values and those deduced by others using entirely different means (e.g. broad-band spectroscopy or imaging) gives us confidence in the reliability of the diagnostics. Two of the SNRs, Puppis A and N132D, show evidence for an overabundance of oxygen by factors of three or more. These results, based on a handful of weak lines, show the great promise of the much more powerful future spectroscopy missions for revealing detailed information about astrophysical plasmas.

Type
4. Supernova Remnants, Soft X-ray Background
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990 , pp. 136 - 145
Copyright
Copyright © Cambridge University Press 1990

References

Canizares, C.R. and Winkler, P.F. 1981, Ap. J., 246, L33.Google Scholar
Canizares, C.R., Winkler, P. F., Markert, T. H., and Berg, C. 1983, in Danziger, J. and Gorenstein, P. (eds), Supernova Remnants and Their X-ray Emission, (Reidel), 205.Google Scholar
Dwek, E., Petre, R., Szymkowiak, A., and Rice, W. L. 1987, Ap. J., 320, 27.Google Scholar
Fabian, A. C., Willingale, R., Pye, J. P., Murray, S. S., and Fabbiano, G. 1980, M. N. R. A. S., 193, 175.Google Scholar
Gabriel, A., Bely-Dubau, F., Faucher, P., and Acton, L. 1988, Ap. J. (in press).Google Scholar
Gabriel, A. and Jordan, C. 1969, M.N.R.A.S., 145, 241.Google Scholar
Giacconi, R. 1979, Ap. J., 230, 540.Google Scholar
Gorenstein, P., Harnden, R., and Tucker, W. 1974, Ap. J., 192, 661.CrossRefGoogle Scholar
Hamilton, A. and Sarazin, C. 1984, Ap. J., 284, 60.Google Scholar
Hamilton, A., Sarazin, C., and Chevalier, R. 1983, Ap. J. Supp., 51, 115.Google Scholar
Hughes, J. 1987, Ap. J., 314, 103.CrossRefGoogle Scholar
Hughes, J. and Helfand, D. 1985, Ap. J., 291, 544.CrossRefGoogle Scholar
Itoh, H., 1977, Pub. Astron. Soc. Japan, 29, 813.Google Scholar
Jansen, F. 1988, Ph.D. Thesis, Leiden State University, The Netherlands.Google Scholar
Jansen, F., Smith, A., Bleeker, J. A. M., de Korte, P. A. J., Peacock, A., and White, N. E. 1988, Ap. J., 331,949.CrossRefGoogle Scholar
Kallne, E. et al. 1984, Phys. Rev. Lett., 52, 2245.Google Scholar
Lasker, B. 1980, Ap. J., 237,765.CrossRefGoogle Scholar
Markert, T.H., Canizares, C.R., Clark, G.W., and Winkler, P.F. 1983, Ap. J., 268, 134.Google Scholar
Markert, T., Blizzard, P., Canizares, C., and Hughes, J. 1988a, in Roger, R. S.and Landecker, T. L.(eds) Supernova Remnants and the Interstellar Medium, (Cambridge Univ. Press), 129.Google Scholar
Markert, T., Blizzard, P., Canizares, C., and Hughes, J. 1988b, in preparation.Google Scholar
Mewe, R., Gronenschild, E. H. B. M., and van den Oord, G. H. J. 1985, Astron. Ap. Supp., 62, 197.Google Scholar
Mewe, R. and Schrijver, J. 1978, Astron. Ap., 65, 99.Google Scholar
Prahdan, A. 1983, Phys. Rev. A., 28,2128.Google Scholar
Petre, R., Canizares, C.R., Kriss, G.A., and Winkler, P.F. 1981, Ap. J., 258, 22.Google Scholar
Szymkowiak, A. E. 1985, NASA Tech. Memorandum 86169.Google Scholar
Tsunemi, H., Manabe, M., Yamashita, K., and Koyama, K. 1988, Publ. Astron. Soc. Japan, 40, 449.Google Scholar
Winkler, P.F. Canizares, C.R., Clark, G.W., Markert, T.H., and Petre, R. 1981, Ap. J., 245, 574.Google Scholar
Winkler, P.F., Tuttle, J.H., Kirshner, R.P. and Irwin, M.J. 1988, in Supernova Remnants and the Interstellar Medium, eds. Roger, R.S. and Landecker, T.L., (Cambridge University Press, Cambridge 65.)Google Scholar
Zarnecki, J. C., Culhane, J. J., Toor, A., Seward, F. D., and Charles, P. A. 1978, Ap. J. (Letters), 219, L17.CrossRefGoogle Scholar