Dynamics of line-driven disk winds

D. Proga

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arXiv · astro-ph/0109092

Dynamics of line-driven disk winds

D. Proga

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Abstract

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.

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D. Proga. 2001-09-06. Dynamics of line-driven disk winds. https://arxiv.org/abs/astro-ph/0109092

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