Gas Cooling Processes

Gas Cooling Processes is a physical mechanism within the broader class of energy dissipation phenomena in interstellar media, distinguished by the emission of infrared and submillimeter radiation from atoms and molecules in photodissociated gas that results from far-ultraviolet radiation-induced excitation and subsequent radiative decay, thereby reducing the thermal energy of the region.

459

Publications

37.8K

Citations

1.2K

Authors

468

Institutions

Publications per year

2017–2026

75

Authors

1.2K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    21 publications · 2.3K citations

    18

    h-index

  2. CS
    Carlos S. Frenk

    Durham University, United Kingdom

    10 publications · 2K citations

    10

    h-index

  3. BR
    B. R. McNamara

    University of Waterloo, Canada

    9 publications · 462 citations

    9

    h-index

  4. CL
    Craig L. Sarazin

    University of Virginia, United States

    8 publications · 363 citations

    8

    h-index

  5. JS
    Joop Schaye

    Leiden University, Netherlands

    8 publications · 1.6K citations

    8

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 125 publications · 13.5K citations

    58

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    117 publications · 10K citations

    54

    h-index

  3. Astronomy and Astrophysics

    35 publications · 1.6K citations

    24

    h-index

  4. The Astrophysical Journal Letters

    10 publications · 440 citations

    10

    h-index

  5. 8

    h-index

1–5