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

Publications

13.2K

Citations

404

Authors

229

Institutions

Publications per year

2017–2026

144

Authors

404

  1. BB
    Bertram Bitsch

    Max Planck Institute for Astronomy, Germany

    22 publications · 2.3K citations

    22

    h-index

  2. AJ
    Anders Johansen

    Lund University, Sweden

    23 publications · 3.8K citations

    20

    h-index

  3. ML
    Michiel Lambrechts

    Lund University, Sweden

    14 publications · 3.3K citations

    14

    h-index

  4. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    11 publications · 1.5K citations

    11

    h-index

  5. CW
    Chris W. Ormel

    University of Amsterdam, Netherlands

    8 publications · 443 citations

    8

    h-index

1–5 of 404

Venues

  1. Astronomy and Astrophysics

    67 publications · 6.4K citations

    39

    h-index

  2. 19

    h-index

  3. The Astrophysical Journal

    ApJ · 22 publications · 715 citations

    18

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 12 publications · 958 citations

    12

    h-index

  5. arXiv (Cornell University)

    Repository · 7 publications · 378 citations

    7

    h-index

1–5