Thick Disk Accretion
Thick Disk Accretion is a theoretical model of accretion processes in which the accreting plasma forms a geometrically thick, optically thin, radiation-inefficient structure around a compact object, distinguished from thin disk models by its pressure-supported vertical equilibrium and advective energy transport.
93
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6K
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371
Authors
214
Institutions
Publications per year
2017–2026
9
Parents
93
On the nature of FU Orionis objects
Lee Hartmann, Scott J. Kenyon · The Astrophysical Journal · 1985 · 292 citations
Natural Sciences, Astronomy, Physics +15
Thin, thick and dark discs in ΛCDM
Justin I. Read, George Lake, Oscar Agertz et al. · Monthly Notices of the Royal Astronomical Society · 2008 · 288 citations · Full text
Natural Sciences, Astronomy, Physics +14
Thick accretion disks and supercritical luminosities.
B. Paczyński, Paul J. Wiita · 1979 · 225 citations
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Goddard Space Flight Center
Greenbelt, United States
7 h-index
10 publications
892 citations
California Institute of Technology
Pasadena, United States
6 h-index
9 publications
431 citations
Nicolaus Copernicus Astronomical Center
Warsaw, Poland
5 h-index
6 publications
238 citations
Institute of Space and Astronautical Science
Tokyo, Japan
5 h-index
16 publications
2.2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
7 publications
693 citations
The University of Tokyo
Tokyo, Japan
5 h-index
13 publications
338 citations

Space Telescope Science Institute
Baltimore, United States
4 h-index
9 publications
1.2K citations

Pennsylvania State University
State College, United States
4 h-index
14 publications
2.2K citations
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ApJ · 44 publications · 3K citations
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12 publications · 1.1K citations
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8 publications · 444 citations
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4 publications · 226 citations
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PRD · 3 publications · 74 citations
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