Molecular Cooling

Molecular Cooling is a radiative process in which excited molecules in interstellar or circumstellar environments release energy through photon emission, thereby reducing their internal and translational kinetic energy within astrophysical gas systems.

278

Publications

17.4K

Citations

716

Authors

264

Institutions

Publications per year

2017–2026

60

Authors

716

  1. JM
    John M. Doyle

    Harvard University, United States

    14 publications · 1.5K citations

    13

    h-index

  2. DC
    D. Comparat

    Laboratoire Aimé Cotton, France

    10 publications · 332 citations

    10

    h-index

  3. PW
    Pepijn W. H. Pinkse

    Max Planck Institute of Quantum Optics, Germany

    6 publications · 288 citations

    6

    h-index

  4. GM
    Gerard Meijer

    Fritz Haber Institute of the Max Planck Society, Germany

    6 publications · 812 citations

    6

    h-index

  5. JT
    Jonathan Tennyson

    University College London, United Kingdom

    6 publications · 280 citations

    6

    h-index

1–5 of 716

Venues

  1. Physical Review A

    PRA · 27 publications · 1.3K citations

    22

    h-index

  2. Physical Review Letters

    PRL · 22 publications · 2.1K citations

    21

    h-index

  3. The Astrophysical Journal

    ApJ · 22 publications · 1.8K citations

    19

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    20 publications · 1.3K citations

    18

    h-index

  5. 13

    h-index

1–5