Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...256..693m&link_type=abstract
Astrophysical Journal, Part 1, vol. 256, May 15, 1982, p. 693-705.
Astronomy and Astrophysics
Astrophysics
18
Binary Stars, Stellar Mass Accretion, Stellar Winds, Supercritical Flow, X Ray Astronomy, Astrophysics, Novae, Optical Thickness, Quasars, Stellar Models, Thermal Emission
Scientific paper
The thermal structure and emergent spectral properties of the supereritical winds outlined in Paper II are presented. Thermal emission due to free-free and Compton processes is considered, along with some nonthermal aspects, for the case when the photons are untrapped throughout the wind envelope. Useful figures and procedures for determining the injection region temperature, emergent spectral temperature, and rough spectral shape are outlined with some attention given to models with central objects of 1 Msun and 108 Msun. A scenario is outlined where the central source of quasars is interpreted as a supercritical wind heated at its base on a nearly dynamical time scale.
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