Protostellar Rotation

Protostellar Rotation is the rotational motion of a protostar, characterized by the angular momentum-driven spinning of the collapsing molecular cloud core during early stellar formation, distinguishing it from subsequent rotational evolution phases in pre-main-sequence and main-sequence stars.

47

Publications

3K

Citations

217

Authors

125

Institutions

Publications per year

2017–2026

8

Authors

217

  1. PT
    Paul T. P. Ho

    Center for Astrophysics Harvard & Smithsonian, United States

    5 publications · 524 citations

    5

    h-index

  2. QZ
    Qizhou Zhang

    Center for Astrophysics Harvard & Smithsonian, United States

    4 publications · 320 citations

    4

    h-index

  3. CL
    Chin‐Fei Lee

    Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan

    4 publications · 327 citations

    4

    h-index

  4. NH
    Naomi Hirano

    Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan

    4 publications · 427 citations

    4

    h-index

  5. FB
    F. Bacciotti

    Arcetri Astrophysical Observatory, Italy

    3 publications · 76 citations

    3

    h-index

1–5 of 217

Venues

  1. The Astrophysical Journal

    ApJ · 27 publications · 1.7K citations

    23

    h-index

  2. 6

    h-index

  3. Astronomy and Astrophysics

    4 publications · 302 citations

    4

    h-index

  4. The Astrophysical Journal Letters

    3 publications · 86 citations

    3

    h-index

  5. Icarus

    1 publications · 16 citations

    1

    h-index

1–5