Hostname: page-component-669899f699-rg895 Total loading time: 0 Render date: 2025-04-27T11:06:46.595Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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

References

Braun, R., 1985. Ph.D. Thesis,, Univ. of Leiden.Google Scholar
Draine, B.T., 1981. Astrophys. J., 245, 880.Google Scholar
Inoue, H., Koyama, K., and Tanaka, Y., 1983. Supernova Remnants and their X-ray Emission, (ed. Danziger, J. and Gorenstein, P.) Reidel, Dordrecht p. 535.Google Scholar
Raymond, J.C., 1984. Ann. Rev. Astr. Astrophys., 22, 75.CrossRefGoogle Scholar
Blair, W.P., Krishner, R.P., and Winkler, P.F., 1983. Astrophys. J., 272, 84.Google Scholar
Blair, W.P., Raymond, J.C., Fesen, R.A., and Gull, T.R., 1984. Astrophys. J., 279, 708.CrossRefGoogle Scholar