Type I Planetary Migration

Type I Planetary Migration is a type of orbital migration in planetary systems wherein a low-mass planet undergoes rapid drift through a protoplanetary disk due to gravitational torques arising from interactions with the surrounding gas, distinguishing it from higher-mass-driven migration mechanisms by its linear response regime and lack of significant disk gap formation.

61

Publications

3.6K

Citations

75

Authors

89

Institutions

Publications per year

2017–2026

18

Authors

75

  1. RE
    Ralph E. Pudritz

    McMaster University, Canada

    4 publications · 222 citations

    4

    h-index

  2. DN
    D. N. C. Lin

    University of California, Santa Cruz, United States

    3 publications · 202 citations

    3

    h-index

  3. YH
    Yasuhiro Hasegawa

    Jet Propulsion Laboratory, United States

    3 publications · 175 citations

    3

    h-index

  4. BB
    Bertram Bitsch

    Max Planck Institute for Astronomy, Germany

    2 publications · 35 citations

    2

    h-index

  5. FM
    F. Masset

    Universidad Nacional Autónoma de México, Mexico

    2 publications · 66 citations

    2

    h-index

1–5 of 75

Venues

  1. The Astrophysical Journal

    ApJ · 18 publications · 1.2K citations

    16

    h-index

  2. Astronomy and Astrophysics

    12 publications · 1.1K citations

    12

    h-index

  3. 10

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 6 publications · 307 citations

    6

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 2 publications · 113 citations

    2

    h-index

1–5