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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

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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

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