Molecular Cloud Core Collapse

Molecular Cloud Core Collapse is a physical astrophysical process in protostellar evolution wherein a gravitationally unstable region within a molecular cloud undergoes contraction due to self-gravity, initiating the formation of a protostar by dissipating thermal and magnetic support mechanisms.

207

Publications

17.8K

Citations

234

Authors

154

Institutions

Publications per year

2017–2026

20

Authors

234

  1. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    18 publications · 953 citations

    15

    h-index

  2. MR
    Matthew R. Bate

    University of Exeter, United Kingdom

    12 publications · 1.8K citations

    12

    h-index

  3. TM
    Tomoaki Matsumoto

    Hosei University, Japan

    8 publications · 837 citations

    8

    h-index

  4. KT
    Kohji Tomisaka

    National Astronomical Observatory of Japan, Japan

    7 publications · 809 citations

    7

    h-index

  5. DJ
    Daniel J. Price

    Monash University, Australia

    6 publications · 716 citations

    6

    h-index

1–5 of 234

Venues

  1. The Astrophysical Journal

    ApJ · 95 publications · 8.7K citations

    52

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    41 publications · 3.9K citations

    30

    h-index

  3. Astronomy and Astrophysics

    10 publications · 603 citations

    11

    h-index

  4. The Astrophysical Journal Letters

    5 publications · 287 citations

    5

    h-index

  5. 4

    h-index

1–5