Photoionized Regions Around Supernova Remnants

Details Photoionized Regions Around Supernova Remnants Photoionized Regions Around Supernova Remnants

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.281..267a&link_type=abstract

Astrophysics and Space Science, v. 281, Issue 1, p. 267-270 (2002).

Astronomy and Astrophysics

Astrophysics

Radiative Transfer, Shock Waves, Supernova Remnants

Scientific paper

The radiation produced by the gas cooling behind a fast supernova remnant shock in the interstellar medium is capable of ionizing the undisturbed medium ahead of the shock wave. In this work I investigate the nonequilibrium evolution of these photoionized precursor regions by means of radiation-hydrodynamic simulations of supernova remnant evolution.

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