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Non-Equilibrium Condition in the SNR

Published online by Cambridge University Press:  25 May 2016

H. Tsunemi
H. Tsunemi*
Affiliation:
Graduate School of Science, Osaka University 1-1 Machikaneyama-cho, Toyonaka, Osaka 560, Japan

Extract

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SNe are one of the major source of the heavy elements in Galaxy. They produced high temperature plasma heavily contaminated with heavy elements mixing with the interstellar matter. Due to the temperature and the density, the shock heated plasma does not reach the collisional ionization condition in young SNR, like Cassiopeia A, Tycho and Kepler. The emission is well represented with a non-equilibrium condition plasma.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 39 - 42
Copyright
Copyright © Kluwer 1998 

References

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