Protostellar Evolution

Protostellar Evolution is the astrophysical process comprising the gravitational collapse of a molecular cloud core and the subsequent accretion-driven growth of a protostar, distinguished from other stages of star formation by its characteristic energy generation through infall and contraction rather than nuclear fusion.

619

Publications

54K

Citations

1.1K

Authors

446

Institutions

Publications per year

2017–2026

127

Authors

1.1K

  1. JK
    J. K. Jørgensen

    University of Copenhagen, Denmark

    21 publications · 1.5K citations

    19

    h-index

  2. EI
    Eduard I. Vorobyov

    University of Vienna, Austria

    19 publications · 1.1K citations

    16

    h-index

  3. KO
    Kazuyuki Omukai

    Tohoku University, Japan

    16 publications · 3.2K citations

    15

    h-index

  4. JT
    John Tobin

    National Radio Astronomy Observatory, United States

    14 publications · 746 citations

    14

    h-index

  5. MN
    Masahiro N. Machida

    Kyushu University, Japan

    14 publications · 1.1K citations

    14

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 226 publications · 24.6K citations

    88

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    112 publications · 10.5K citations

    52

    h-index

  3. Astronomy and Astrophysics

    102 publications · 6.5K citations

    48

    h-index

  4. The Astrophysical Journal Letters

    14 publications · 694 citations

    14

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 17 publications · 582 citations

    14

    h-index

1–5