Interstellar Gas Accretion

Interstellar Gas Accretion is a theoretical astrophysical process denoting the gravitationally driven capture and accumulation of diffuse interstellar gas by celestial bodies or galactic structures, distinguished from other gas dynamics mechanisms by its role in fueling star formation and galaxy evolution through the continuous inflow of external baryonic matter.

275

Publications

26.8K

Citations

784

Authors

390

Institutions

Publications per year

2017–2026

72

Authors

784

  1. FF
    Filippo Fraternali

    University of Groningen, Netherlands

    7 publications · 936 citations

    7

    h-index

  2. VS
    Volker Springel

    Max Planck Institute for Astrophysics, Germany

    6 publications · 4.1K citations

    6

    h-index

  3. RM
    R. Maiolino

    University of Cambridge, United Kingdom

    5 publications · 391 citations

    5

    h-index

  4. JW
    Jing Wang

    Peking University, China

    4 publications · 316 citations

    4

    h-index

  5. JS
    Joseph Silk

    University of Oxford, United Kingdom

    4 publications · 292 citations

    4

    h-index

1–5 of 784

Venues

  1. The Astrophysical Journal

    ApJ · 89 publications · 9K citations

    49

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    89 publications · 9.8K citations

    48

    h-index

  3. Astronomy and Astrophysics

    20 publications · 1.6K citations

    17

    h-index

  4. The Astronomical Journal

    AJ · 12 publications · 771 citations

    12

    h-index

  5. 8

    h-index

1–5