Environmental Quenching

Environmental quenching is a astrophysical process in which external environmental factors, such as ram pressure stripping, tidal interactions, or galaxy harassment in dense cluster environments, suppress star formation in dwarf galaxies by removing or disrupting their gas reservoirs, thereby distinguishing it from internal quenching mechanisms driven by stellar or black hole feedback.

56

Publications

3.2K

Citations

313

Authors

194

Institutions

Publications per year

2017–2026

42

Authors

313

  1. MC
    Michael C. Cooper

    University of California, Irvine, United States

    12 publications · 690 citations

    12

    h-index

  2. GW
    Gillian Wilson

    University of California, Riverside, United States

    10 publications · 449 citations

    10

    h-index

  3. RF
    R. F. J. van der Burg

    European Southern Observatory, Germany

    10 publications · 407 citations

    10

    h-index

  4. AM
    Adam Muzzin

    York University, Canada

    10 publications · 449 citations

    10

    h-index

  5. RD
    R. Demarco

    University of Concepción, Chile

    9 publications · 375 citations

    9

    h-index

1–5 of 313

Venues

  1. Monthly Notices of the Royal Astronomical Society

    26 publications · 1.5K citations

    22

    h-index

  2. The Astrophysical Journal

    ApJ · 15 publications · 977 citations

    16

    h-index

  3. Astronomy and Astrophysics

    3 publications · 171 citations

    3

    h-index

  4. The Astrophysical Journal Letters

    2 publications · 161 citations

    2

    h-index

  5. Lancaster EPrints (Lancaster University)

    Repository · 1 publications · 152 citations

    1

    h-index

1–5