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IRAS Observations of Collisionally Heated Dust in Large Magellanic Cloud Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

James R. Graham ,
A. Evans ,
J.S. Albinson ,
M.F. Bode  and
W.P.S. Meikle
James R. Graham
Affiliation:
Imperial College, London Lawrence Berkeley Laboratory, University of California
A. Evans
Affiliation:
University of Keele
J.S. Albinson
Affiliation:
University of Keele
M.F. Bode
Affiliation:
Lancashire Polytechnic
W.P.S. Meikle
Affiliation:
Imperial College, London

Abstract

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IRAS additional observations show that luminous (104−105 L⊙) far-IR sources are associated with the Large Magellanic Cloud (LMC) supernova remnants N63A, N49, N49B, and N186D. Comparison of the IRAS and X-ray data shows that a substantial fraction of the IR emission from three of the SNRs can be accounted for by collisionally heated dust. The ratio of dust-grain cooling to total atomic cooling is ~10 in X-ray emitting gas (T~106 K). We show why dust cooling does not dominate, but probably speeds SNR evolution in an inhomogeneous interstellar medium.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 383 - 386
Copyright
Copyright © Cambridge University Press 1988

References

Draine, B.T., & Salpeter, E.E. 1979, Ap. J., 231, 77.CrossRefGoogle Scholar
Gatley, I., Becklin, E.E., Werner, M.W., & Wynn-Williams, C.G. 1977, Ap. J., 216, 277.Google Scholar
Graham, J.R., Evans, A., Albinson, J.S., Bode, M.F., & Meikle, W.P.S. 1987, Ap. J., 319, 000 Google Scholar
Graham, J.R., Wright, G.S., & Longmore, A.J., 1987, Ap. J., 313, 847.CrossRefGoogle Scholar
Harvey, P.M., Hoffmann, W.F., & Campbell, M.F. 1979 Ap. J., 227, 114.CrossRefGoogle Scholar
Harvey, P.M., Campbell, M.F., & Hoffmann, W.F. 1979 Ap. J., 228, 445.CrossRefGoogle Scholar
Harvey, P.M., Thronson, H.A., & Gatley, I. 1979, Ap. J., 231, 115.CrossRefGoogle Scholar
Lequeux, J., Peimbert, M., Rayo, J.F., Serrano, A., & Torres-Peimbert, S. 1979, Astr. Ap. 80, 55.Google Scholar
Mathewson, D.S., Ford, V.L., Dopita, M.A., Tuohy, I.R., Long, K.S., & Helfand, D.J. 1983, Ap. J Suppl. Ser., 51, 345.Google Scholar
Ostriker, J.P., & Silk, J. 1973, Ap. J. Lett, 184, L113.Google Scholar
Raymond, J.C., Cox, D.P., & Smith, B.W. 1976, Ap. J., 204, 290.Google Scholar
Spitzer, L. 1978, Physical Processes in the Interstellar Medium, Wiley, New York.Google Scholar