Structure of Radiative Shock Waves in Stellar Atmospheres |
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| Authors: | Yu.A. Fadeyev D. Gillet |
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| Affiliation: | (1) Institute for Astronomy of the Russian Academy of Sciences, Pyatnitskaya 48, 109017 Moscow, Russia;(2) Observatoire de Haute-Provence - CNRS, F-04870 Saint-Michel l'Observatoire, France |
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| Abstract: | A global iteration method to determine the self-consistent structure of steady plane-parallel radiative shock waves is shown to converge to the stable solution with upstream front velocities of 15 km/s ≤ U 1≤ 60 km/s and for hydrogen gas of unperturbed temperature T= 3000 K and density ρ = 10−10gcm−3. This revised version was published online in July 2006 with corrections to the Cover Date. |
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