Radiative shocks in atomic and molecular stellar-like atmospheres. VII. Influence of the excited level of the hydrogen atom: the wake structure

Details Radiative shocks in atomic and molecular stellar-like atmospheres. VII. Influence of the excited level of the hydrogen atom: the wake structure Radiative shocks in atomic and molecular stellar-like atmospheres. VII. Influence of the excited level of the hydrogen atom: the wake structure

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...290..518h&link_type=abstract

Astronomy and Astrophysics 290, 518-530 (1994)

Astronomy and Astrophysics

Astrophysics

2

Shock Waves, Stars: Atmospheres, Stars: Agb And Post-Agb

Scientific paper

We investigate the structure of a steady state monodimensional radiative shock wave propagating through a collisional hydrogen gas composed of both atoms and molecules. The framework of this study is a "three mean photons model" taking into account the Lyman and Balmer continua and the Lyman-α line at the same time. The ambient conditions (1000K

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