The Influence of Hydrodynamical Winds on Hot Accretion Disk Solutions
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/553/i=2/a=978/pdf
Reference36 articles.
1. Accretion Disks Phase Transitions: 2-D or Not 2-D?
2. On the absence of winds in advection-dominated accretion flows
3. Instability, turbulence, and enhanced transport in accretion disks
4. Advection‐dominated Accretion with Infall and Outflows
5. Magnetic Field Limitations on Advection‐dominated Flows
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2. VISCOUS ACCRETION OF A POLYTROPIC SELF-GRAVITATING DISK IN THE PRESENCE OF WIND;The Astrophysical Journal;2013-02-21
3. ON THE STRUCTURE OF ACCRETION DISKS WITH OUTFLOWS;The Astrophysical Journal;2011-05-13
4. Thermally Driven Winds from Radiatively Inefficient Accretion Flows;Publications of the Astronomical Society of Japan;2009-10-25
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