Accretion Disk Winds
Accretion Disk Winds is a physical phenomenon in accretion physics characterized by the outflow of ionized gas or plasma from the surface layers of an accretion disk, driven by radiation pressure, magnetic forces, or thermal effects, thereby removing mass, angular momentum, and energy from the disk system.
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358
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Accretion Disk Winds from Active Galactic Nuclei
Norman Murray, J. Chiang, Scott A. Grossman et al. · The Astrophysical Journal · 1995 · 869 citations
Natural Sciences, Astronomy, Physics +17
The AGN-obscuring Torus: The End of the "Doughnut" Paradigm?
Moshe Elitzur, Isaac Shlosman · The Astrophysical Journal · 2006 · 493 citations · Full text
Natural Sciences, Astronomy, Physics +14
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Goddard Space Flight Center
Greenbelt, United States
23 h-index
53 publications
5.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
23 h-index
45 publications
3.2K citations
University of Maryland, College Park
College Park, United States
21 h-index
35 publications
4.8K citations
University of Nevada, Las Vegas
Las Vegas, United States
17 h-index
26 publications
1.3K citations
University of Oxford
Oxford, United Kingdom
15 h-index
22 publications
1.6K citations

Centre National de la Recherche Scientifique
Paris, France
15 h-index
59 publications
3.8K citations
University of Cambridge
Cambridge, United Kingdom
13 h-index
21 publications
858 citations
Deleted Institution
12 h-index
31 publications
2K citations
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ApJ · 121 publications · 12.1K citations
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