Thermal instability behind a radiative shock

Details Thermal instability behind a radiative shock Thermal instability behind a radiative shock

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979afz....15..347s&link_type=abstract

(Astrofizika, vol. 15, Apr.-June 1979, p. 347-354.) Astrophysics, vol. 15, no. 2, Oct. 1979, p. 224-228. Translation.

Astronomy and Astrophysics

Astrophysics

2

Astrophysics, Radiative Transfer, Shock Fronts, Thermal Instability, Adiabatic Conditions, H Ii Regions, Hydrogen Ions, Shock Wave Propagation, Wave Excitation

Scientific paper

The possibility of thermal instability behind a shock front with
de-excitation is investigated. The conditions for the adiabatic mode of
thermal instability are the most favorable. It is possible that
precisely this mode leads to the formation of inhomogeneities in the
neighborhood of compact H II regions.

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