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.

68

Publications

5.4K

Citations

90

Authors

81

Institutions

Publications per year

2017–2026

21

Authors

90

  1. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    6 publications · 315 citations

    6

    h-index

  2. AC
    A. Crida

    Observatoire de la Côte d’Azur, France

    5 publications · 259 citations

    5

    h-index

  3. RP
    Richard P. Nelson

    Queen Mary University of London, United Kingdom

    5 publications · 338 citations

    5

    h-index

  4. BB
    Bertram Bitsch

    Max Planck Institute for Astronomy, Germany

    4 publications · 130 citations

    4

    h-index

  5. WK
    W. Kley

    University of Tübingen, Germany

    3 publications · 65 citations

    3

    h-index

1–5 of 90

Venues

  1. The Astrophysical Journal

    ApJ · 20 publications · 2.3K citations

    19

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    19 publications · 1.2K citations

    16

    h-index

  3. Astronomy and Astrophysics

    12 publications · 835 citations

    11

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 5 publications · 276 citations

    5

    h-index

  5. arXiv (Cornell University)

    Repository · 2 publications · 52 citations

    2

    h-index

1–5