Collapse Timescales

Collapse Timescales is a theoretical construct in astrophysics that denotes the characteristic duration required for a self-gravitating molecular cloud or protostellar core to undergo gravitational collapse under its own gravity, distinguishing it from other dynamical timescales by specifically quantifying the free-fall or near-free-fall evolution toward hydrostatic equilibrium in star-forming regions.

109

Publications

7.9K

Citations

246

Authors

171

Institutions

Publications per year

2017–2026

20

Authors

246

  1. UD
    Ujjal Debnath

    Indian Institute of Engineering Science and Technology, Shibpur, India

    3 publications · 73 citations

    3

    h-index

  2. FH
    Fabian Heitsch

    University of North Carolina at Chapel Hill, United States

    3 publications · 236 citations

    3

    h-index

  3. SC
    Subenoy Chakraborty

    Jadavpur University, India

    3 publications · 73 citations

    3

    h-index

  4. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    2 publications · 169 citations

    2

    h-index

  5. NG
    N. G. Parker

    Newcastle University, United Kingdom

    2 publications · 114 citations

    2

    h-index

1–5 of 246

Venues

  1. The Astrophysical Journal

    ApJ · 13 publications · 972 citations

    12

    h-index

  2. 9

    h-index

  3. General Relativity and Gravitation

    6 publications · 128 citations

    6

    h-index

  4. Physical Review Letters

    PRL · 5 publications · 427 citations

    5

    h-index

  5. Astronomy and Astrophysics

    4 publications · 266 citations

    4

    h-index

1–5