Diagnostics of Supernova Remnant Shock Waves

Details Diagnostics of Supernova Remnant Shock Waves Diagnostics of Supernova Remnant Shock Waves

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.233..231r&link_type=abstract

Astrophysics and Space Science, Volume 233, Issue 1-2, pp. 231-237

Astronomy and Astrophysics

Astrophysics

2

Shock Waves, Supernova Remnants

Scientific paper

Fairly simple models can explain the emission from non-radiative shock waves in supernova remnants. This talk reviews some of the more robust diagnostics of shock parameters and some of the implications for the physics of collisionless shock waves in interstellar gas. The Hopkins Ultraviolet Telescope observed several non-radiative shocks during the ASTRO-2 mission, and the spectra have interesting implications for the physics of collisionless shocks.

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