A distribution function calculation of the H α profiles of SNR filaments

Details A distribution function calculation of the H α profiles of SNR filaments A distribution function calculation of the H α profiles of SNR filaments

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.233..273l&link_type=abstract

Astrophysics and Space Science, Volume 233, Issue 1-2, pp. 273-280

Astronomy and Astrophysics

Astrophysics

Supernova Remnants, Shock Waves

Scientific paper

In shocked media of high preshock ionisation, the lack of thermal contact between atoms in the neutral component of the gas can prevent the formation of a thermal equilibrium independent of the ionic component. The behaviour of the neutral gas in such a shock is dominated by the atomic processes driven by the postshock ionic component. A transport equation for the velocity distribution of the neutral gas is explicitly solved under the physical conditions of a 1D ionic shock transition. The resulting distributions are used to calculate predicted H α line emission from such a system.

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