Galaxy Quenching

Galaxy Quenching is the astrophysical process by which star formation in a galaxy is suppressed or terminated, distinguishing it from ongoing star-forming galaxies through the cessation of cold gas conversion into stars due to internal or environmental mechanisms.

175

Publications

13.1K

Citations

714

Authors

304

Institutions

Publications per year

2017–2026

136

Authors

714

  1. RM
    R. Maiolino

    University of Cambridge, United Kingdom

    11 publications · 703 citations

    11

    h-index

  2. ST
    Sandro Tacchella

    University of Cambridge, United Kingdom

    9 publications · 547 citations

    9

    h-index

  3. MC
    Michael C. Cooper

    University of California, Irvine, United States

    9 publications · 608 citations

    9

    h-index

  4. RD
    Romeel Davé

    University of the Western Cape, South Africa

    7 publications · 1.1K citations

    9

    h-index

  5. MB
    Michael Boylan-Kolchin

    The University of Texas at Austin, United States

    7 publications · 497 citations

    7

    h-index

1–5 of 714

Venues

  1. Monthly Notices of the Royal Astronomical Society

    65 publications · 6.2K citations

    39

    h-index

  2. The Astrophysical Journal

    ApJ · 37 publications · 3.5K citations

    28

    h-index

  3. The Astrophysical Journal Letters

    12 publications · 648 citations

    12

    h-index

  4. Astronomy and Astrophysics

    8 publications · 443 citations

    10

    h-index

  5. arXiv (Cornell University)

    Repository · 7 publications · 162 citations

    8

    h-index

1–5