Protostellar Initial Conditions

Protostellar Initial Conditions is a theoretical construct in astrophysics that specifies the physical and chemical starting parameters—such as mass, temperature, density, and angular momentum—of a collapsing molecular cloud core from which a protostar forms, distinguishing it from subsequent evolutionary states by representing the initial boundary conditions for star formation models.

79

Publications

7.2K

Citations

173

Authors

137

Institutions

Publications per year

2017–2026

6

Authors

173

  1. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    6 publications · 218 citations

    6

    h-index

  2. HW
    H. W. Yorke

    Jet Propulsion Laboratory, United States

    5 publications · 758 citations

    5

    h-index

  3. SW
    Steven W. Stahler

    University of California, Berkeley, United States

    4 publications · 527 citations

    4

    h-index

  4. KO
    Kazuyuki Omukai

    Tohoku University, Japan

    4 publications · 1.3K citations

    4

    h-index

  5. DW
    D. Ward–Thompson

    Cardiff University, United Kingdom

    4 publications · 586 citations

    4

    h-index

1–5 of 173

Venues

  1. The Astrophysical Journal

    ApJ · 30 publications · 4.6K citations

    28

    h-index

  2. 12

    h-index

  3. Astronomy and Astrophysics

    9 publications · 562 citations

    9

    h-index

  4. ArXiv.org

    Repository · 3 publications · 76 citations

    3

    h-index

  5. arXiv (Cornell University)

    Repository · 2 publications · 62 citations

    2

    h-index

1–5