Cool Gas Clouds

Cool Gas Clouds is a construct in astrophysics referring to discrete, gravitationally unbound reservoirs of ionized or neutral interstellar medium observed within the circumgalactic medium, distinguished by their relatively low temperatures (typically 10^4 K or below) and high column densities of metal ions, which facilitate the study of gas accretion, feedback, and phase structure in galaxy halos.

276

Publications

18.6K

Citations

811

Authors

328

Institutions

Publications per year

2017–2026

65

Authors

811

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    10 publications · 545 citations

    10

    h-index

  2. SP
    S. Peng Oh

    University of California, Santa Barbara, United States

    9 publications · 1.3K citations

    10

    h-index

  3. RL
    R. L. Snell

    University of Massachusetts Amherst, United States

    6 publications · 426 citations

    6

    h-index

  4. MG
    Max Grönke

    Max Planck Institute for Astrophysics, Germany

    5 publications · 308 citations

    5

    h-index

  5. GM
    G. Mark Voit

    Michigan State University, United States

    5 publications · 350 citations

    5

    h-index

1–5 of 811

Venues

  1. The Astrophysical Journal

    ApJ · 119 publications · 8.6K citations

    50

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    70 publications · 5.5K citations

    35

    h-index

  3. Astronomy and Astrophysics

    9 publications · 579 citations

    9

    h-index

  4. Nature

    7 publications · 563 citations

    7

    h-index

  5. The Astronomical Journal

    AJ · 6 publications · 277 citations

    6

    h-index

1–5