Dynamical models of radiative shocks. I - Steady shocks

Details Dynamical models of radiative shocks. I - Steady shocks Dynamical models of radiative shocks. I - Steady shocks

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.224..179i&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 224, Jan. 1, 1987, p. 179-192. Research supported by th

Physics

Atomic Physics

31

Dynamic Models, Interstellar Radiation, Ion Atom Interactions, Radiation Distribution, Shock Waves, Atomic Physics, Collisional Plasmas, High Temperature, Steady Flow

Scientific paper

The ionization structure and line emission behind a steady radiative shock are calculated with a consistent treatment of the radiation field and the shock precursor. The results agree well with those of previous authors, except that the Hβ intensity is about twice that found in earlier calculations. Only relatively low velocity shocks are considered, since, as will be shown in later papers, high velocity shocks are unstable and unlikely to be steady.

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