Protostellar Heating

Protostellar Heating is a physical process in star formation whereby gravitational energy is converted into thermal energy within a collapsing molecular cloud core, leading to the gradual increase in temperature and pressure that characterizes the early evolution of a protostar.

39

Publications

2.4K

Citations

207

Authors

123

Institutions

Publications per year

2017–2026

11

Authors

207

  1. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    9 publications · 666 citations

    9

    h-index

  2. LE
    L. E. Kristensen

    Leiden University, Netherlands

    5 publications · 551 citations

    5

    h-index

  3. SD
    S. D. Doty

    Denison University, United States

    5 publications · 529 citations

    5

    h-index

  4. JK
    J. K. Jørgensen

    University of Copenhagen, Denmark

    4 publications · 412 citations

    4

    h-index

  5. DJ
    Doug Johnstone

    Herzberg Institute of Astrophysics, Canada

    4 publications · 419 citations

    4

    h-index

1–5 of 207

Venues

  1. The Astrophysical Journal

    ApJ · 8 publications · 610 citations

    8

    h-index

  2. 7

    h-index

  3. Astronomy and Astrophysics

    7 publications · 332 citations

    7

    h-index

  4. The Astrophysical Journal Letters

    3 publications · 171 citations

    3

    h-index

  5. arXiv (Cornell University)

    Repository · 2 publications · 127 citations

    2

    h-index

1–5