Disk-driven Migration

Disk-Driven Migration is a type of planetary migration mechanism in which gravitational interactions between a planet and the surrounding protoplanetary disk result in the net transfer of angular momentum, thereby causing the planet to undergo orbital evolution within the disk.

76

Publications

8.6K

Citations

177

Authors

129

Institutions

Publications per year

2017–2026

25

Authors

177

  1. JA
    John Asher Johnson

    University of California, Berkeley, United States

    4 publications · 1.5K citations

    4

    h-index

  2. SP
    Sijme-Jan Paardekooper

    University of Cambridge, United Kingdom

    4 publications · 494 citations

    4

    h-index

  3. FC
    Fred C. Adams

    University of Michigan, United States

    3 publications · 200 citations

    3

    h-index

  4. WK
    W. Kley

    University of Tübingen, Germany

    3 publications · 71 citations

    3

    h-index

  5. RI
    Rebekah I. Dawson

    Pennsylvania State University, United States

    3 publications · 625 citations

    3

    h-index

1–5 of 177

Venues

  1. The Astrophysical Journal

    ApJ · 24 publications · 2.4K citations

    22

    h-index

  2. Astronomy and Astrophysics

    13 publications · 1.4K citations

    12

    h-index

  3. The Astrophysical Journal Letters

    10 publications · 1.8K citations

    9

    h-index

  4. 8

    h-index

  5. The Astronomical Journal

    AJ · 7 publications · 450 citations

    7

    h-index

1–5