Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-08T05:07:14.507Z Has data issue: false hasContentIssue false

Non-Equilibrium Thermal X-Ray Emission in the Early Phase of Supernova Remnant

Published online by Cambridge University Press:  14 August 2015

Hitoshi Hanami
Affiliation:
Department of Physics, I.F.S., University of Texas, Austin, TX 78712–1060
Tatsuo Yoshida
Affiliation:
Department of Physics, Hokkaido University, Sapporo 060, Japan

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 X-ray emission from the interaction of the ejecta with circumstellar matter (CSM) for SN1987A is investigated. The electron and the ion temperatures seem to be in non-equilibrium in the early phase of a SN remnant. We have studied the two-temperature model in the early phase of SNR and discuss the X-ray emission from SN1987A and its CSM.

Type
Joint Discussions
Copyright
Copyright © Kluwer 1989

References

Chevalier, R.A. 1982, Astrophys.J. 258, 790.Google Scholar
Chevalier, R.A. and Fransson, C. 1987, Nature 328, 44.Google Scholar
Colgate, S.A. and McKee, C. 1969, Astrophys.J. 157, 623.Google Scholar
Cox, D.P. and Anderson, P.R. 1982, Astrophys.J. 253, 263.Google Scholar
Dotani, T. et al. 1987, Nature 330, 230.Google Scholar
Gilmozzi, R. et al. 1987, Nature 328, 318.Google Scholar
Hanami, H. and Sakashita, S. 1987, Astron. Astrophys. 181, 343.Google Scholar
Itoh, H. 1978, Publ.Astron.Soc.Japan 30, 489.Google Scholar
Itoh, H. 1979, Publ.Astron.Soc.Japan 31, 429E.Google Scholar
Itoh, H., Hayakawa, S., Masai, K., and Nomoto, K. 1987, Publ. As tr. Soc. Japan 39, 529.Google Scholar
Itoh, H. et al. 1987, Nature, 330, 233.Google Scholar
Masai, S., Hayakawa, S., Itoh, H. and Nomoto, K. 1987, Nature 330, 233.Google Scholar
Turtle, A.J. et al. 1987, Nature, 329, 38.Google Scholar