Interstellar Gas Heating

Interstellar Gas Heating is a physical process in astrophysics whereby energy from stellar radiation, cosmic rays, and turbulent motions is transferred to the diffuse interstellar medium, increasing the thermal energy of its gaseous components through photoionization, collisional excitation, and other microscopic interactions.

141

Publications

11.8K

Citations

360

Authors

234

Institutions

Publications per year

2017–2026

29

Authors

360

  1. DJ
    D. J. Hollenbach

    Ames Research Center, United States

    4 publications · 1.6K citations

    4

    h-index

  2. DG
    Donald Goldsmith

    Stanford University, United States

    4 publications · 963 citations

    4

    h-index

  3. JS
    Joseph Silk

    University of Oxford, United Kingdom

    3 publications · 115 citations

    3

    h-index

  4. AD
    A. Dalgarno

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 69 citations

    3

    h-index

  5. RM
    Richard McCray

    Joint Institute for Laboratory Astrophysics, United States

    3 publications · 155 citations

    3

    h-index

1–5 of 360

Venues

  1. The Astrophysical Journal

    ApJ · 72 publications · 7.5K citations

    40

    h-index

  2. 15

    h-index

  3. Astronomy and Astrophysics

    10 publications · 451 citations

    10

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 3 publications · 54 citations

    3

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 2 publications · 130 citations

    2

    h-index

1–5