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Possibilities for Observations with the Infrared Space Observatory of Emission from Shock–Heated Dust in SNRs

Published online by Cambridge University Press:  12 April 2016

J. Svestka
J. Svestka*
Affiliation:
Prague Observatory, Prague, Czechoslovakia*

Abstract

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The possibilities for observing infrared emission from shock-heated dust in SNRs with the future Infrared Space Observatory (ISO) are illustrated with calculations of the ISOPHOT-P and ISOPHOT-C flux densities and integration times for radiation from six selected SNRs in eight wavelength bands between 4µm and 180µm.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 387 - 390
Copyright
Copyright © Cambridge University Press 1988

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