Type I Planetary Migration
Type I Planetary Migration is a type of orbital migration in planetary systems wherein a low-mass planet undergoes rapid drift through a protoplanetary disk due to gravitational torques arising from interactions with the surrounding gas, distinguishing it from higher-mass-driven migration mechanisms by its linear response regime and lack of significant disk gap formation.
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75
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89
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2017–2026
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Halting type I planet migration in non-isothermal disks
Astronomy and Astrophysics · 2006 · 294 citations · Full text
Planet migration in three-dimensional radiative discs
W. Kley, B. Bitsch, Hubert Klahr · Astronomy and Astrophysics · 2009 · 183 citations · Full text
Migration of protoplanets in radiative discs
W. Kley, A. Crida · Astronomy and Astrophysics · 2008 · 176 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Centre National de la Recherche Scientifique
Paris, France
12 h-index
25 publications
1.2K citations
University of California, Santa Cruz
Santa Cruz, United States
6 h-index
6 publications
490 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
5 h-index
9 publications
333 citations
Tokyo Institute of Technology
Tokyo, Japan
5 h-index
7 publications
540 citations

Sorbonne Université
Paris, France
4 h-index
10 publications
276 citations
Observatoire de la Côte d’Azur
Nice, France
4 h-index
6 publications
307 citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
4 h-index
4 publications
263 citations
University of Michigan
Ann Arbor, United States
4 h-index
7 publications
450 citations
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ApJ · 18 publications · 1.2K citations
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12 publications · 1.1K citations
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10 publications · 326 citations
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Repository · 6 publications · 307 citations
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Repository · 2 publications · 113 citations
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