Hostname: page-component-cc8bf7c57-n7qbj Total loading time: 0 Render date: 2024-12-12T07:42:19.959Z Has data issue: false hasContentIssue false
  • English
  • Français

Thermal and Non-Thermal X-Rays from SN 1006 and IC 443

Published online by Cambridge University Press:  25 May 2016

M. Ozaki  and
K. Koyama
M. Ozaki
Affiliation:
The Institute of Space and Astronautical Science, 3-1-1, Yoshinodai, Sagamihara, Kanagawa, 229, Japan
K. Koyama
Affiliation:
Department of Physics, Faculty of Science, Kyoto University, Kitashirakawa, Sakyo, Kyoto, 606-01, Japan

Extract

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.

From many Galactic supernova remnants (SNRs), X-ray emissions consisting of non-equilibrium ionization (NEI) plasma and additional hard component are detected. The hard emission have been usually interpreted as a high temperature plasma of = 10 keV. However, the recent observation with ASCA made it clear that the hard components of some SNRs are of non-thermal origin. Here we report the ASCA results of SN 1006 and IC 443 observations as an example of such SNRs.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 256 - 257
Copyright
Copyright © Kluwer 1998 

References

1. Asaoka, I. and Aschenbach, B. 1994, AA, 284, 573 Google Scholar
2. Koyama, K., Petre, R., Gotthelf, E. V., Hwang, U., Matsuura, M., Ozaki, M. and Holt, S. S. 1995, Nature, 378, 255 CrossRefGoogle Scholar
3. Petre, R., Szymkowiak, A. E., Seward, F. D. and Willingale, R. 1988, ApJ, 335, 214 Google Scholar