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An Infrared Survey of Galactic Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

Richard G. Arendt
Richard G. Arendt*
Affiliation:
University of Illinois, 349 Astronomy Bldg., 1011 W. Springfield, Urbana, IL 61801

Abstract

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Presented here are preliminary results from a survey of supernova remnants (SNRs) in the data base collected by the Infrared Astronomical Satellite (IRAS). About one-third of the known galactic SNRs are visible in the IRAS data. Confusion with other sources in the galactic plane prohibits the detection of many remnants. The objects that are detected have similar spectral characteristics and temperatures, except that the three youngest remnants known, Tycho, Kepler, and Cassiopeia A, are distinctly warmer.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 379 - 382
Copyright
Copyright © Cambridge University Press 1988

References

Antonopoulou, E., and Pottasch, S.R., 1987, Astr. Ap., 173, 108.Google Scholar
Chini, R., Kreysa, E., Mezger, P.G., and Gemünd, H.-P., 1986, Astr. Ap., 154, 8.Google Scholar
Dwek, E., 1981, Ap. J., 247, 614.Google Scholar
IRAS Catalogs and Atlases, Explanatory Supplement 1985, edited by Beichman, C.A., Neugebauer, G., Habing, H.J., Clegg, P.E., and Chester, T.J., (Washington D.C.: U. S. Government Printing Office.)Google Scholar
Pottasch, S.R., Baud, B., Beintema, D., Emerson, J., Habing, H.J., Harris, S., Houck, J., Jennings, R., and Marsden, P., 1984, Astr. Ap., 138, 10.Google Scholar