Multiphase Gas Structure

Multiphase Gas Structure is a theoretical construct in astrophysics that denotes the coexistence of thermally distinct gaseous phases—spanning cold, warm, and hot temperature regimes—within the circumgalactic medium, distinguished by their ionization states, densities, and dynamical interactions that govern galaxy feedback and accretion processes.

159

Publications

12.6K

Citations

492

Authors

299

Institutions

Publications per year

2017–2026

81

Authors

492

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    7 publications · 1.1K citations

    7

    h-index

  2. CF
    Claude‐André Faucher‐Giguère

    Northwestern University, United States

    6 publications · 318 citations

    6

    h-index

  3. LH
    Lars Hernquist

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 996 citations

    6

    h-index

  4. NW
    Norbert Werner

    Kavli Institute for Particle Astrophysics and Cosmology, United States

    6 publications · 397 citations

    6

    h-index

  5. JS
    J. S. Sanders

    Max Planck Institute for Extraterrestrial Physics, Germany

    5 publications · 943 citations

    5

    h-index

1–5 of 492

Venues

  1. The Astrophysical Journal

    ApJ · 57 publications · 5.3K citations

    36

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    62 publications · 4.9K citations

    35

    h-index

  3. Astronomy and Astrophysics

    7 publications · 485 citations

    7

    h-index

  4. The Astrophysical Journal Letters

    6 publications · 445 citations

    6

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 3 publications · 86 citations

    3

    h-index

1–5