Pebble Accretion
Pebble Accretion is a planetary formation mechanism in which centimeter- to meter-sized solid particles in a protoplanetary disk are gravitationally captured by growing planetary embryos, enabling rapid mass growth through aerodynamic drag-induced orbital decay.
213
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13.2K
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404
Authors
229
Institutions
Publications per year
2017–2026
144
213
Rapid growth of gas-giant cores by pebble accretion
Astronomy and Astrophysics · 2012 · 854 citations · Full text
Natural Sciences, Astronomy, Physics +16
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Lund University
Lund, Sweden
26 h-index
67 publications
11.2K citations

Centre National de la Recherche Scientifique
Paris, France
24 h-index
50 publications
5.3K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
24 h-index
68 publications
4.7K citations
Observatoire de la Côte d’Azur
Nice, France
16 h-index
21 publications
2.4K citations
Tokyo Institute of Technology
Tokyo, Japan
15 h-index
30 publications
1.7K citations
University of Bern
Bern, Switzerland
15 h-index
36 publications
2K citations
Life Science Institute
Tokyo, Japan
13 h-index
21 publications
944 citations

Université Côte d'Azur
Nice, France
12 h-index
16 publications
2.1K citations
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67 publications · 6.4K citations
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27 publications · 1K citations
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ApJ · 22 publications · 715 citations
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Repository · 12 publications · 958 citations
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Repository · 7 publications · 378 citations
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