Class 0 Protostars

Class 0 Protostar is a young stellar object in the earliest observational stage of protostellar evolution, distinguished by a centrally condensed core embedded within a dense infalling envelope, where the majority of luminosity arises from accretion and envelope emission rather than stellar photospheric emission.

240

Publications

15.8K

Citations

642

Authors

302

Institutions

Publications per year

2017–2026

66

Authors

642

  1. JT
    John Tobin

    National Radio Astronomy Observatory, United States

    22 publications · 1.3K citations

    22

    h-index

  2. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    20 publications · 2K citations

    20

    h-index

  3. JK
    J. K. Jørgensen

    University of Copenhagen, Denmark

    17 publications · 2.1K citations

    17

    h-index

  4. TL
    Tyler L. Bourke

    Center for Astrophysics Harvard & Smithsonian, United States

    15 publications · 1.6K citations

    15

    h-index

  5. SM
    S. Maret

    Centre National de la Recherche Scientifique, France

    15 publications · 1.1K citations

    15

    h-index

1–5 of 642

Venues

  1. The Astrophysical Journal

    ApJ · 80 publications · 5.6K citations

    43

    h-index

  2. Astronomy and Astrophysics

    62 publications · 4.9K citations

    40

    h-index

  3. The Astrophysical Journal Letters

    10 publications · 550 citations

    10

    h-index

  4. arXiv (Cornell University)

    Repository · 10 publications · 408 citations

    10

    h-index

  5. The Astrophysical Journal Supplement Series

    9 publications · 869 citations

    9

    h-index

1–5