Non-Equilibrium Thermal X-ray Emission in the Early Phase of Supernova Remnant
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.
KeywordsElectron Temperature Contact Discontinuity Radio Observation Simple Analytic Method Thermal Bremsstrahlung
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