Type Ii Planetary Migration
Type II Planetary Migration is a mode of orbital evolution in which a massive planet opens a gap in the protoplanetary disk and migrates inward due to gravitational interactions with the disk material, with the migration rate governed by the disk's viscous evolution.
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2017–2026
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Max Planck Institute for Astronomy
Heidelberg, Germany
8 h-index
14 publications
1.1K citations
Queen Mary University of London
London, United Kingdom
7 h-index
11 publications
1.2K citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
22 publications
1.3K citations
Observatoire de la Côte d’Azur
Nice, France
6 h-index
20 publications
848 citations

Lund University
Lund, Sweden
5 h-index
8 publications
669 citations

University of Tübingen
Tübingen, Germany
5 h-index
12 publications
569 citations
Canadian Institute for Theoretical Astrophysics
Toronto, Canada
4 h-index
4 publications
183 citations
University of Cambridge
Cambridge, United Kingdom
3 h-index
4 publications
93 citations
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ApJ · 20 publications · 2.3K citations
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19 publications · 1.2K citations
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12 publications · 835 citations
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Repository · 5 publications · 276 citations
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Repository · 2 publications · 52 citations
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