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Non-Equilibrium Thermal X-Ray Emission in the Early Phase of Supernova Remnant
Published online by Cambridge University Press: 14 August 2015
Abstract
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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.
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- Copyright © Kluwer 1989
References
Itoh, H., Hayakawa, S., Masai, K., and Nomoto, K.
1987, Publ. As tr. Soc. Japan
39, 529.Google Scholar
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