Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-28T02:31:10.955Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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

References

Arnaud, M., and Rothenflug, R., 1985, Astron.Astroph.Suppl. 60, p. 425.Google Scholar
Brinkmann, W., and Fink, H.H., 1987, in preparationGoogle Scholar
Chevalier, R.A., 1982, Ap.J. 259, L59.CrossRefGoogle Scholar
Gorenstein, P., Seward, F., and Tucker, W., 1983, Proc. IAU Symposium 101 Google Scholar
Hamilton, A.J.S., Sarazin, C.L., and Szymkowiak, A.E., 1986 Ap. J. 300, p. 713 Google Scholar
Nomoto, K., Thielemann, F.K., and Yokoi, K., 1984, Ap.J. 286, p. 644 Google Scholar
Tsunemi, H., Yamashita, K., Masai, K., and Hayakawa, S., 1986 Ap. J. 306, p. 21.CrossRefGoogle Scholar
Wilkins, M.L., 1980, J. Comp. Phys. 36, p. 281.Google Scholar