Line-driven winds from accretion disks. I - Effects of the ionization structure

Details Line-driven winds from accretion disks. I - Effects of the ionization structure Line-driven winds from accretion disks. I - Effects of the ionization structure

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...327..680v&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 327, April 15, 1988, p. 680-692. Research supported by Science Applications

Statistics

Computation

34

Accretion Disks, Black Holes (Astronomy), Galactic Nuclei, Ionization Cross Sections, Stellar Luminosity, Stellar Winds, Active Galaxies, Cataclysmic Variables, Computational Astrophysics, Early Stars, Hot Stars

Scientific paper

The authors have investigated both analytically and numerically the basic characteristics of line-driven winds from UV accretion disks. Stellar winds have been compared with the outflow from a disk surrounding a supermassive black hole. The authors find that in the approximation of vertically streaming radiation close to the disk photosphere, the existence of steady disk winds depends crucially on their ionization structure, a basic difference when compared to the stellar winds. The necessary criteria for the line radiation force to support the disk wind are presented and discussed.

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