Resonant Planetary Migration

Resonant Planetary Migration is a theoretical framework in planetary system dynamics that describes the coupled orbital evolution of planets due to gravitational interactions with a protoplanetary disk, distinguished by the capture and sustained evolution of planets in mean-motion resonance.

180

Publications

12.7K

Citations

249

Authors

189

Institutions

Publications per year

2017–2026

58

Authors

249

  1. CB
    C. Beaugé

    Universidad Nacional de Córdoba, Argentina

    10 publications · 502 citations

    10

    h-index

  2. SN
    Sean N. Raymond

    Laboratoire d'Astrophysique de Bordeaux, France

    10 publications · 1.4K citations

    10

    h-index

  3. BB
    Bertram Bitsch

    Max Planck Institute for Astronomy, Germany

    9 publications · 1.1K citations

    9

    h-index

  4. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    8 publications · 1.5K citations

    8

    h-index

  5. CM
    Cezary Migaszewski

    Nicolaus Copernicus University, Poland

    7 publications · 260 citations

    7

    h-index

1–5 of 249

Venues

  1. Monthly Notices of the Royal Astronomical Society

    53 publications · 3.1K citations

    29

    h-index

  2. The Astrophysical Journal

    ApJ · 24 publications · 2.8K citations

    21

    h-index

  3. Astronomy and Astrophysics

    27 publications · 1.8K citations

    21

    h-index

  4. The Astronomical Journal

    AJ · 22 publications · 1.3K citations

    19

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 9 publications · 408 citations

    9

    h-index

1–5