Disk-driven Migration
Disk-Driven Migration is a type of planetary migration mechanism in which gravitational interactions between a planet and the surrounding protoplanetary disk result in the net transfer of angular momentum, thereby causing the planet to undergo orbital evolution within the disk.
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2017–2026
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HOT STARS WITH HOT JUPITERS HAVE HIGH OBLIQUITIES
Joshua N. Winn, Daniel C. Fabrycky, Simon Albrecht et al. · The Astrophysical Journal Letters · 2010 · 744 citations · Full text
Natural Sciences, Astronomy, Physics +13
Rebekah I. Dawson, John Asher Johnson · Annual Review of Astronomy and Astrophysics · 2018 · 589 citations · Full text
Natural Sciences, Astronomy, Physics +17
Accretion during the Merger of Supermassive Black Holes
The Astrophysical Journal · 2002 · 406 citations · Full text
Natural Sciences, Astronomy, Physics +17
Halting type I planet migration in non-isothermal disks
Astronomy and Astrophysics · 2006 · 294 citations · Full text
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
8 h-index
20 publications
2.7K citations
California Institute of Technology
Pasadena, United States
8 h-index
12 publications
1.4K citations
Queen Mary University of London
London, United Kingdom
6 h-index
12 publications
1.8K citations
Massachusetts Institute of Technology
Cambridge, United States
6 h-index
15 publications
2K citations

University of Tübingen
Tübingen, Germany
6 h-index
12 publications
493 citations
NASA Exoplanet Science Institute
Pasadena, United States
5 h-index
7 publications
1.1K citations

Centre National de la Recherche Scientifique
Paris, France
5 h-index
11 publications
1.1K citations
University of Cambridge
Cambridge, United Kingdom
5 h-index
6 publications
822 citations
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ApJ · 24 publications · 2.4K citations
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13 publications · 1.4K citations
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10 publications · 1.8K citations
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8 publications · 318 citations
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AJ · 7 publications · 450 citations
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