Galaxy Environment Effects

Galaxy Environment Effects is a theoretical construct in astrophysics that identifies how the large-scale structure and local density of the cosmic web—such as clusters, filaments, and voids—modulate the star formation rates, morphologies, and evolutionary pathways of galaxies through processes like ram pressure stripping, galaxy harassment, and tidal interactions, distinguishing it from intrinsic galaxy evolution mechanisms driven by internal processes.

721

Publications

55.7K

Citations

2.3K

Authors

638

Institutions

Publications per year

2017–2026

222

Authors

2.3K

  1. LV
    L. Verdes‐Montenegro

    Instituto de Astrofísica de Andalucía, Spain

    18 publications · 957 citations

    17

    h-index

  2. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    17 publications · 862 citations

    16

    h-index

  3. JS
    J. Sabater

    Royal Observatory, United Kingdom

    15 publications · 842 citations

    15

    h-index

  4. LT
    L. Tresse

    Laboratoire d’Astrophysique de Marseille, France

    15 publications · 3.7K citations

    15

    h-index

  5. LC
    L. Cortese

    International Centre for Radio Astronomy Research, Australia

    16 publications · 1K citations

    15

    h-index

1–5 of 2.3K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    273 publications · 19.6K citations

    74

    h-index

  2. The Astrophysical Journal

    ApJ · 173 publications · 15.9K citations

    62

    h-index

  3. Astronomy and Astrophysics

    93 publications · 5.4K citations

    43

    h-index

  4. The Astronomical Journal

    AJ · 28 publications · 3.1K citations

    21

    h-index

  5. The Astrophysical Journal Letters

    12 publications · 916 citations

    12

    h-index

1–5