High-frequency Radio Continuum

High-Frequency Radio Continuum is a type of radio continuum emission characterized by its origination in the high-frequency end of the radio spectrum, typically above a few gigahertz, and distinguished by its predominance of non-thermal processes such as synchrotron radiation and reduced influence from thermal bremsstrahlung and interstellar scintillation effects.

228

Publications

9.5K

Citations

1K

Authors

358

Institutions

Publications per year

2017–2026

22

Authors

1K

  1. MT
    M. Tornikoski

    University of Turku, Finland

    8 publications · 477 citations

    8

    h-index

  2. HD
    H. D. Aller

    University of Michigan, United States

    7 publications · 411 citations

    7

    h-index

  3. MF
    M. F. Aller

    University of Michigan, United States

    7 publications · 444 citations

    7

    h-index

  4. AL
    A. Lähteenmäki

    Aalto University, Finland

    6 publications · 352 citations

    6

    h-index

  5. LF
    Luis F. Rodrı́guez

    Universidad Nacional Autónoma de México, Mexico

    5 publications · 278 citations

    5

    h-index

1–5 of 1K

Venues

  1. The Astrophysical Journal

    ApJ · 43 publications · 2K citations

    25

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    33 publications · 1.8K citations

    20

    h-index

  3. The Astronomical Journal

    AJ · 26 publications · 976 citations

    18

    h-index

  4. Astronomy and Astrophysics

    23 publications · 861 citations

    17

    h-index

  5. Nature

    14 publications · 581 citations

    13

    h-index

1–5