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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

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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.

Information

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

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