Protostellar Disks

Protostellar Disks is a rotating circumstellar disk of gas and dust gravitationally bound to a forming protostar, through which mass is transported inward toward the central object while angular momentum is redistributed outward, enabling accretion and stellar growth during the early stages of star formation.

621

Publications

58.6K

Citations

1.2K

Authors

473

Institutions

Publications per year

2017–2026

167

Authors

1.2K

  1. ZL
    Zhi‐Yun Li

    University of Virginia, United States

    29 publications · 2.1K citations

    23

    h-index

  2. DN
    D. N. C. Lin

    University of California, Santa Cruz, United States

    20 publications · 4.7K citations

    20

    h-index

  3. JT
    John Tobin

    National Radio Astronomy Observatory, United States

    20 publications · 1.5K citations

    19

    h-index

  4. JK
    J. K. Jørgensen

    University of Copenhagen, Denmark

    20 publications · 1.5K citations

    19

    h-index

  5. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    17 publications · 2.4K citations

    17

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 280 publications · 27.6K citations

    91

    h-index

  2. Astronomy and Astrophysics

    89 publications · 6.1K citations

    43

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    62 publications · 3.6K citations

    36

    h-index

  4. The Astrophysical Journal Letters

    24 publications · 1.1K citations

    20

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 14 publications · 816 citations

    13

    h-index

1–5