Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-12T15:50:36.741Z Has data issue: false hasContentIssue false
  • English
  • Français

Infrared Analysis of Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

Eli Dwek
Eli Dwek*
Affiliation:
Laboratory for Astronomy and Solar Physics, NASA/Goddard Space Flight Center, Maryland

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.

Infrared observations of supernova remnants obtained with the Infrared Astronomical Satellite provide new insights into the dynamics and energetics of the remnants, and into their interaction with the ambient interstellar medium. In most remnants the infrared emission arises from dust that is collisionally heated by the X-ray emitting gas. The infrared observations can therefore be used as a diagnostic for the physical conditions of the shocked gas. In particular, it is shown that all the prominent X-ray remnants in the Galaxy and in the LMC cool mainly by dust grain collisions instead of atomic processes.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 363 - 378
Copyright
Copyright © Cambridge University Press 1988

References

Arendt, R.G. 1987a, this volume.Google Scholar
Arendt, R.G. 1987b, private communications.Google Scholar
Braun, R. 1986a, Astr. Ap., 162, 259.Google Scholar
Braun, R. 1986b, Astr. Ap., 164, 193.Google Scholar
Braun, R. 1986c, Astr. Ap., 164, 208.Google Scholar
Braun, R. 1987, Astr. Ap., 171, 233.Google Scholar
Burke, J.R., and Silk, J. 1974, Ap. J., 190, 1.Google Scholar
Caswell, J.L. 1987, this volume.Google Scholar
Chevalier, R.A. 1974, Ap. J., 188, 501.CrossRefGoogle Scholar
Cox, D.P. 1972, Ap. J., 178, 159.Google Scholar
Dinerstein, H.L., Lester, D.F., Rank, D.M., Werner, M.W., and Wooden, D.H. 1987, Ap. J., 312, 314.Google Scholar
Draine, B.T. 1981, Ap. J., 245, 880.Google Scholar
Draine, B.T., and Salpeter, E.E. 1979a, Ap. J. 231, 77.CrossRefGoogle Scholar
Draine, B.T., and Salpeter, E.E. 1979b, Ap. J., 231, 438.Google Scholar
Draine, B.T., and Anderson, N. 1985, Ap. J., 292, 494.CrossRefGoogle Scholar
Dwek, E. 1981, Ap. J., 247, 614 Google Scholar
Dwek, E., and Werner, M.W. 1981, Ap. J., 248, 138 Google Scholar
Dwek, E. 1986, Ap. J., 302, 363 Google Scholar
Dwek, E., Dinerstein, H.L., Gillett, F.C., Hauser, M.G., and Rice, W.L. 1987a, Ap. J., 315, 571.Google Scholar
Dwek, E. 1987, Ap. J., in press.Google Scholar
Dwek, E., Petre, R., Szymkowiak, A., and Rice, W.L. 1987b, AD. J. (Letters), in press.Google Scholar
Graham, J.R., Evans, A., Albinson, J.S., Bode, M.F., and Meikle, W.P.S. 1987, Ap. J., 319, 000 Google Scholar
Hamilton, A.J.S., Sarazin, C.L., and Chevalier, R.A. 1983, Ap. J. Suppl. 51, 115 (HSC).Google Scholar
Harvey, P.M., Gatley, I., and Thronson, H.A. 1978, Pub. A. S. P., 90, 143 Google Scholar
Hauser, M.G., et al. 1984, Ap. J. (letters). 278, 15.Google Scholar
Ku, W.H.-M., Kahn, S.M., Pisarski, R.L., and Long, K.S. 1984, Ap. J., 278, 615 CrossRefGoogle Scholar
Low, F.J., et al. 1984, Ap. J. (letters). 278, 19.Google Scholar
Marsden, P.L., Gillett, F.C., Jennings, R.E., Emerson, J.P., de Jong, T., Olnon, F.M. 1984, Ap. J. (Letters), 278, 29.Google Scholar
Mathis, J.S., Rumpl, W., and Nordsieck, K.H. 1977. Ap. J., 217, 425 Google Scholar
Matsui, Y., Long, K.S., Dickel, J.R., and Greisen, E.W. 1984, Ap. J., 287, 295 Google Scholar
McCollough, M.L., and Mufson, S.L. 1987, this volume.Google Scholar
McKee, C.F. 1987, this volume.Google Scholar
Mezger, P.G., Tuffs, R.J., Chini, R., Kreysa, E., and Gemund, H.-P. 1986, Astr. Ap., 167, 145 Google Scholar
Mufson, S.L., McCollough, M.L., Dickel, J.R., Petre, R., White, R., and Chevalier, R. 1986, A. J., 92, 1349.Google Scholar
Murray, S.S., Fabbiano, G., Fabian, A.C., Epstein, A., and Giacconi, R. 1979, Ap. J. (Letters). 234, 69.Google Scholar
Neugebauer, G. et al. 1984, Ap. J. (Letters). 278, L1.Google Scholar
Ostriker, J.P., and Silk, J. 1973, Ap. J. (Letters), 184, L113.Google Scholar
Pisarski, R.L., Helfand, D.J., and Kahn, S.M. 1984, Ap. J., 277, 710 Google Scholar
Pottash, S.R. 1984, Planetary Nebulae (Dordrecht: Reidel), page 302.Google Scholar
Raymond, J.C., Cox, D.P., and Smith, B.W. 1976, Ap. J., 204, 290 CrossRefGoogle Scholar
Seab, C.G. 1986, Interstellar Processes, eds. Hollenbach, D., and Thronson, H.A. Jr. (Dordrecht: Reidel).Google Scholar
Seward, F., Gorenstein, P., and Tucker, W. 1983, Ap. J., 266, 287 CrossRefGoogle Scholar
Shull, J.M. 1977, Ap. J., 215, 805 Google Scholar
Shull, J.M. 1980, Ap. J., 237, 769 Google Scholar
Silk, J., and Burke, J.R. 1974, Ap. J., 190, 11.Google Scholar
Spitzer, L. 1978, Physical Processes in the Interstellar Medium (New York: Interscience), p. 199.Google Scholar
Weiland, J.L., Blitz, L., Dwek, E., Hauser, M.G., Magnani, L., and Rickard, J.L. 1986, Ap. J. (Letters), 306, 101.CrossRefGoogle Scholar
Wheeler, J.C., Mazurek, T.J., and Sivaramakrishnan, A. 1980, Ap. J., 237, 781.Google Scholar
Wright, E.L., Harper, D.A., Lowenstein, R.F., Keene, J., and Whitcomb, S.E. 1980, Ap. J. (Letters). 240, L157.Google Scholar