Interstellar Gas Cooling

Interstellar Gas Cooling is a physical process in astrophysics whereby thermal energy is radiated away from low-density gas in the diffuse interstellar medium through atomic and molecular line emissions, thereby reducing the gas temperature and influencing the medium’s thermal balance and dynamical evolution.

255

Publications

22.7K

Citations

525

Authors

284

Institutions

Publications per year

2017–2026

30

Authors

525

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    17 publications · 2.2K citations

    15

    h-index

  2. WG
    William G. Mathews

    University of California, Santa Cruz, United States

    9 publications · 441 citations

    9

    h-index

  3. FB
    Fabrizio Brighenti

    University of Bologna, Italy

    7 publications · 309 citations

    7

    h-index

  4. CL
    Craig L. Sarazin

    University of Virginia, United States

    7 publications · 296 citations

    7

    h-index

  5. WF
    W. Forman

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 1K citations

    6

    h-index

1–5 of 525

Venues

  1. The Astrophysical Journal

    ApJ · 113 publications · 9.7K citations

    53

    h-index

  2. 39

    h-index

  3. Astronomy and Astrophysics

    17 publications · 865 citations

    15

    h-index

  4. The Astrophysical Journal Supplement Series

    6 publications · 2.1K citations

    6

    h-index

  5. 3

    h-index

1–5