Mass Quenching

Mass quenching is a theoretical mechanism in galactic evolution wherein the cessation of star formation in a galaxy is primarily driven by its stellar mass, distinguishing it from environment-dependent quenching processes.

85

Publications

8.8K

Citations

488

Authors

238

Institutions

Publications per year

2017–2026

47

Authors

488

  1. MF
    Michele Fumagalli

    Durham University, United Kingdom

    8 publications · 549 citations

    8

    h-index

  2. RG
    Riccardo Giovanelli

    Cornell University, United States

    8 publications · 549 citations

    8

    h-index

  3. MP
    Martha P. Haynes

    Cornell University, United States

    8 publications · 549 citations

    8

    h-index

  4. AB
    A. Boselli

    Laboratoire d’Astrophysique de Marseille, France

    8 publications · 549 citations

    8

    h-index

  5. MC
    Michael C. Cooper

    University of California, Irvine, United States

    8 publications · 695 citations

    8

    h-index

1–5 of 488

Venues

  1. Monthly Notices of the Royal Astronomical Society

    38 publications · 3.5K citations

    27

    h-index

  2. The Astrophysical Journal

    ApJ · 17 publications · 3.3K citations

    15

    h-index

  3. Astronomy and Astrophysics

    9 publications · 548 citations

    9

    h-index

  4. Physics Letters B

    2 publications · 202 citations

    2

    h-index

  5. arXiv (Cornell University)

    Repository · 2 publications · 84 citations

    2

    h-index

1–5