Accretion Disks

Accretion Disks is an astrophysical disk structure in star-forming systems that consists of gas and dust in (approximately) Keplerian rotation around a central protostar or young star, through which material transports angular momentum outward and mass inward, thereby mediating stellar growth and setting the initial conditions for planet formation.

8K

Publications

646.2K

Citations

8.7K

Authors

1.7K

Institutions

Publications per year

2017–2026

1.9K

Authors

8.7K

  1. DJ
    David J. Wilner

    Center for Astrophysics Harvard & Smithsonian, United States

    92 publications · 12.5K citations

    57

    h-index

  2. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    92 publications · 14.4K citations

    57

    h-index

  3. LT
    L. Testi

    Arcetri Astrophysical Observatory, Italy

    86 publications · 8.8K citations

    52

    h-index

  4. CP
    C. P. Dullemond

    Max Planck Institute for Astronomy, Germany

    78 publications · 11.2K citations

    51

    h-index

  5. NC
    Nuria Calvet

    University of Michigan, United States

    83 publications · 14.4K citations

    51

    h-index

1–5 of 8.7K

Venues

  1. The Astrophysical Journal

    ApJ · 2.7K publications · 274.3K citations

    229

    h-index

  2. Astronomy and Astrophysics

    1K publications · 73.9K citations

    137

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    1.2K publications · 82.2K citations

    135

    h-index

  4. The Astrophysical Journal Letters

    271 publications · 19.1K citations

    74

    h-index

  5. Nature

    122 publications · 17.9K citations

    72

    h-index

1–5