Disk Cooling
Disk Cooling is a theoretical model that specifies the mechanisms and rates by which thermal energy is radiated away from an accretion disk, thereby reducing its temperature and enabling continued mass inflow through viscous dissipation.
109
Publications
6.9K
Citations
220
Authors
121
Institutions
Publications per year
2017–2026
8
Parents
109
Thermal equilibria of accretion disks
The Astrophysical Journal · 1995 · 595 citations · Full text
Natural Sciences, Astronomy, Physics +17
Nanofluid flow and heat transfer due to a rotating disk
Mustafa Türkyılmazoğlu · Computers & Fluids · 2014 · 477 citations
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220
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121
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
4 h-index
4 publications
432 citations
Institute of Astronomy
Moscow, Russia
3 h-index
3 publications
630 citations
The University of Texas at Austin
Austin, United States
3 h-index
5 publications
102 citations

Centre National de la Recherche Scientifique
Paris, France
3 h-index
15 publications
1.8K citations
University of Illinois Urbana-Champaign
Urbana, United States
3 h-index
5 publications
602 citations
University of Sussex
Brighton, United Kingdom
3 h-index
5 publications
415 citations

Observatoire astronomique de Strasbourg
Strasbourg, France
3 h-index
3 publications
368 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
3 h-index
4 publications
223 citations
1–8 of 121
ApJ · 21 publications · 2K citations
18
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9 publications · 258 citations
9
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7 publications · 336 citations
7
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6 publications · 886 citations
6
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4 publications · 410 citations
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1–5