Accretion Disks
Accretion Disks is an astrophysical disk structure in star-forming systems that consists of gas and dust in (approximately) Keplerian rotation around a central protostar or young star, through which material transports angular momentum outward and mass inward, thereby mediating stellar growth and setting the initial conditions for planet formation.
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Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
James B. Pollack, O. Hubickyj, Peter Bodenheimer et al. · Icarus · 1996 · 3.1K citations
Natural Sciences, Astronomy, Physics +14
Gamma-ray bursts from stellar mass accretion disks around black holes
S. E. Woosley · The Astrophysical Journal · 1993 · 2.5K citations
Natural Sciences, Astronomy, Physics +17
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Center for Astrophysics Harvard & Smithsonian, United States
92 publications · 12.5K citations
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Center for Astrophysics Harvard & Smithsonian, United States
92 publications · 14.4K citations
57
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52
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1.7K
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
141 h-index
1.2K publications
162.6K citations

Centre National de la Recherche Scientifique
Paris, France
120 h-index
2.1K publications
148.8K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
108 h-index
1.2K publications
99.9K citations
California Institute of Technology
Pasadena, United States
102 h-index
551 publications
61.8K citations
Leiden University
Leiden, The Netherlands
96 h-index
630 publications
58.1K citations
University of California, Berkeley
Berkeley, United States
92 h-index
395 publications
48.4K citations
University of Cambridge
Cambridge, United Kingdom
91 h-index
585 publications
42.9K citations
University of Arizona
Tucson, United States
90 h-index
593 publications
49.5K citations
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ApJ · 2.7K publications · 274.3K citations
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1.2K publications · 82.2K citations
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271 publications · 19.1K citations
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122 publications · 17.9K citations
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