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Non-Equilibrium Ionisation in Supernova Remnants - A Case Like Tycho - A case like Tycho

Published online by Cambridge University Press:  12 April 2016

W. Brinkmann  and
H.H. Fink
W. Brinkmann
Affiliation:
Max-Planck-Institut für Physikund Astrophysik, Institut für Extraterrestrische Physik, 8046 Garching, F.R.G.
H.H. Fink
Affiliation:
Max-Planck-Institut für Physikund Astrophysik, Institut für Extraterrestrische Physik, 8046 Garching, F.R.G.

Abstract

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X-ray observations of young supernova remnants (SNR) provide the most direct tool to study their evolution, their chemical composition, and their interaction with the interstellar medium. We will show for a SNR with the characteristics of Tycho that great care has to be taken in interpreting spectral data obtained with X-ray detectors with low spatial resolution.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 137 - 140
Copyright
Copyright © Cambridge University Press 1988

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