Radiative shocks in atomic and molecular stellar-like atmospheres. VIII. A self-consistent comprehensive model.

Details Radiative shocks in atomic and molecular stellar-like atmospheres. VIII. A self-consistent comprehensive model. Radiative shocks in atomic and molecular stellar-like atmospheres. VIII. A self-consistent comprehensive model.

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...324.1046h&link_type=abstract

Astronomy and Astrophysics, v.324, p.1046-1058

Astronomy and Astrophysics

Astrophysics

3

Hydrodynamics, Radiative Transfer, Shock Waves, Circumstellar Matter, Stars: Mass Loss, Stars: Agb, Post-Agb

Scientific paper

This paper is devoted to the modelling of radiative shock waves propagating through a stellar-like atmosphere; that is a collisional atomic and molecular hydrogen gas with temperature and density ranges 1000K

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