Relativistic Jets

Relativistic Jets is a high-energy astrophysical phenomenon consisting of collimated streams of ionized matter accelerated to relativistic speeds along the polar axes of compact objects, typically powered by accretion processes in black hole or neutron star systems within extragalactic X-ray and gamma-ray sources.

1.5K

Publications

109.4K

Citations

4.9K

Authors

1K

Institutions

Publications per year

2017–2026

373

Authors

4.9K

  1. GG
    G. Ghisellini

    Brera Astronomical Observatory, Italy

    27 publications · 4K citations

    22

    h-index

  2. FT
    F. Tavecchio

    Brera Astronomical Observatory, Italy

    27 publications · 2.6K citations

    21

    h-index

  3. MC
    Mitchell C. Begelman

    Joint Institute for Laboratory Astrophysics, United States

    25 publications · 5.3K citations

    21

    h-index

  4. MP
    M. Perucho

    Universitat de València, Spain

    31 publications · 1.4K citations

    21

    h-index

  5. AT
    Alexander Tchekhovskoy

    Northwestern University, United States

    19 publications · 3.3K citations

    19

    h-index

1–5 of 4.9K

Venues

  1. The Astrophysical Journal

    ApJ · 405 publications · 36.4K citations

    100

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    333 publications · 22.6K citations

    77

    h-index

  3. Astronomy and Astrophysics

    134 publications · 7.9K citations

    48

    h-index

  4. The Astrophysical Journal Letters

    53 publications · 3K citations

    30

    h-index

  5. 25

    h-index

1–5