Galactic Continuum Emission

Galactic Continuum Emission is a type of astrophysical radiation process characterized by the broad-spectrum electromagnetic emission originating from interstellar matter and energetic particles within galaxies, distinct from discrete line emission and predominantly arising from mechanisms such as synchrotron radiation, free-free emission, and dust thermal emission.

296

Publications

19.7K

Citations

1.7K

Authors

500

Institutions

Publications per year

2017–2026

51

Authors

1.7K

  1. AW
    A. W. Strong

    Max Planck Institute for Extraterrestrial Physics, Germany

    6 publications · 1.5K citations

    6

    h-index

  2. NM
    N. M. McClure‐Griffiths

    Commonwealth Scientific and Industrial Research Organisation, Australia

    6 publications · 1.1K citations

    6

    h-index

  3. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    5 publications · 951 citations

    5

    h-index

  4. WR
    W. Reich

    Max Planck Institute for Radio Astronomy, Germany

    5 publications · 579 citations

    5

    h-index

  5. KM
    K. M. Menten

    Max Planck Institute for Radio Astronomy, Germany

    5 publications · 237 citations

    5

    h-index

1–5 of 1.7K

Venues

  1. The Astrophysical Journal

    ApJ · 115 publications · 9.2K citations

    50

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    50 publications · 2.7K citations

    29

    h-index

  3. Astronomy and Astrophysics

    29 publications · 1.7K citations

    21

    h-index

  4. The Astrophysical Journal Supplement Series

    9 publications · 798 citations

    9

    h-index

  5. The Astrophysical Journal Letters

    9 publications · 485 citations

    9

    h-index

1–5