2001/09/06 by D. Proga, Daniel Proga, Proga, D.
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #Astrophysical Phenomena and Observations #High-pressure geophysics and materials #Mechanics and Biomechanics Studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0109092
LaTeX, 6 pages, to be published in "Mass Outflow in Active Galactic Nuclei: New Perspectives" eds. D.M.Crenshaw, S.B.Kraemer and I.M.George, ASP Conf. Proc
arxiv created 2001/09/06 · arxiv updated 2009/12/01
I review the main results from recent 2-D, time-dependent hydrodynamic models of radiation-driven winds from accretion disks in AGN. I also discuss the physical conditions needed for a disk wind to be shielded from the strong X-rays and to be accelerated to hypersonic velocities. I conclude with a few remarks on winds in hot stars, low mass young stellar objects, cataclysmic variables, low mass X-ray binaries, and galactic black holes and future work.