Radio Jets

Radio Jet is a high-energy astrophysical phenomenon consisting of collimated streams of relativistic particles and magnetic fields ejected from the vicinity of a supermassive black hole, typically in an active galactic nucleus, and emitting strongly in the radio wavelength regime through synchrotron radiation.

1.7K

Publications

121.9K

Citations

3.8K

Authors

914

Institutions

Publications per year

2017–2026

329

Variants

Radio Jet

Authors

3.8K

  1. MJ
    M. J. Hardcastle

    University of Hertfordshire, United Kingdom

    42 publications · 2.4K citations

    30

    h-index

  2. JA
    J. A. Zensus

    Max Planck Institute for Radio Astronomy, Germany

    44 publications · 3.8K citations

    29

    h-index

  3. RP
    R. P. Fender

    University of Southampton, United Kingdom

    33 publications · 2K citations

    27

    h-index

  4. ER
    E. Ros

    Max Planck Institute for Radio Astronomy, Germany

    34 publications · 3.4K citations

    24

    h-index

  5. JC
    J. C. A. Miller‐Jones

    Curtin University, Australia

    27 publications · 1.5K citations

    23

    h-index

1–5 of 3.8K

Venues

  1. The Astrophysical Journal

    ApJ · 592 publications · 43.8K citations

    107

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    414 publications · 27.9K citations

    77

    h-index

  3. Astronomy and Astrophysics

    183 publications · 9.8K citations

    54

    h-index

  4. The Astronomical Journal

    AJ · 62 publications · 4.6K citations

    36

    h-index

  5. The Astrophysical Journal Letters

    46 publications · 2.4K citations

    29

    h-index

1–5