Emission processes in young SNRs

Details Emission processes in young SNRs Emission processes in young SNRs

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..203r&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 203-212 (2001).

Astronomy and Astrophysics

Astrophysics

Supernova Remnants, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

This paper summarizes the emission processes that produce the radiation we use to study young supernova remnants. We discuss the relative importance of various processes and the accuracy with which the emissivities or rate coefficients are known, especially in cases where uncertainties in the theoretical or laboratory rates may limit the interpretation of observations. Common assumptions that may break down, such as thermal and ionization equilibrium, are discussed. .

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