Interstellar Cooling

Interstellar Cooling is a physical process in astrophysics wherein thermal energy is radiated away from the interstellar medium through electromagnetic emissions, primarily via atomic and molecular line radiation, thereby reducing the gas temperature and regulating star formation and cloud dynamics.

62

Publications

7.6K

Citations

129

Authors

59

Institutions

Publications per year

2017–2026

4

Authors

129

  1. WG
    William G. Mathews

    University of California, Santa Cruz, United States

    4 publications · 99 citations

    4

    h-index

  2. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    4 publications · 1.6K citations

    4

    h-index

  3. FB
    Fabrizio Brighenti

    University of Bologna, Italy

    3 publications · 78 citations

    3

    h-index

  4. RM
    Richard McCray

    Joint Institute for Laboratory Astrophysics, United States

    2 publications · 477 citations

    2

    h-index

  5. DR
    D. R. Flower

    Durham University, United Kingdom

    2 publications · 106 citations

    2

    h-index

1–5 of 129

Venues

  1. The Astrophysical Journal

    ApJ · 37 publications · 3.6K citations

    26

    h-index

  2. 5

    h-index

  3. Astronomy and Astrophysics

    2 publications · 32 citations

    2

    h-index

  4. Annual Review of Astronomy and Astrophysics

    2 publications · 1.3K citations

    2

    h-index

  5. Physical Review

    1 publications · 14 citations

    1

    h-index

1–5