Streaming Instability

Streaming Instability is a hydrodynamic instability in protoplanetary disks that constitutes a theoretical mechanism wherein solid particles and gas interact through drag forces, leading to the spontaneous concentration of solids into dense clumps capable of undergoing gravitational collapse to form planetesimals.

245

Publications

18.5K

Citations

377

Authors

245

Institutions

Publications per year

2017–2026

110

Authors

377

  1. AJ
    Anders Johansen

    Lund University, Sweden

    18 publications · 2.2K citations

    16

    h-index

  2. AN
    Andrew N. Youdin

    University of Arizona, United States

    10 publications · 1.9K citations

    10

    h-index

  3. XB
    Xue‐Ning Bai

    Tsinghua University, China

    8 publications · 887 citations

    8

    h-index

  4. JB
    Jacob B. Simon

    Joint Institute for Laboratory Astrophysics, United States

    8 publications · 772 citations

    8

    h-index

  5. CY
    Chao‐Chin Yang

    University of Nevada, Las Vegas, United States

    7 publications · 651 citations

    7

    h-index

1–5 of 377

Venues

  1. The Astrophysical Journal

    ApJ · 58 publications · 6.3K citations

    37

    h-index

  2. Astronomy and Astrophysics

    39 publications · 3.6K citations

    30

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    38 publications · 1.8K citations

    24

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 14 publications · 1.1K citations

    12

    h-index

  5. The Astrophysical Journal Letters

    10 publications · 785 citations

    10

    h-index

1–5