Gamma-ray Binaries

Gamma-Ray Binaries is a class of high-mass binary star systems in which one component is a compact object that produces persistent and variable gamma-ray emission through particle acceleration and shock interactions in the stellar wind or magnetospheric environment.

246

Publications

13.3K

Citations

2.1K

Authors

455

Institutions

Publications per year

2017–2026

50

Authors

2.1K

  1. GD
    G. Dubus

    Centre National de la Recherche Scientifique, France

    23 publications · 2.3K citations

    21

    h-index

  2. FA
    F. Aharonian

    Max Planck Institute for Nuclear Physics, Germany

    19 publications · 1.4K citations

    17

    h-index

  3. OR
    O. Reimer

    Centre National de la Recherche Scientifique, France

    17 publications · 1.5K citations

    16

    h-index

  4. JM
    J. M. Paredes

    Universitat de Barcelona, Spain

    14 publications · 868 citations

    14

    h-index

  5. AR
    A. Reimer

    Centre National de la Recherche Scientifique, France

    14 publications · 1.4K citations

    14

    h-index

1–5 of 2.1K

Venues

  1. The Astrophysical Journal

    ApJ · 71 publications · 3.3K citations

    32

    h-index

  2. Astronomy and Astrophysics

    39 publications · 2.7K citations

    27

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    33 publications · 1.5K citations

    24

    h-index

  4. The Astrophysical Journal Letters

    22 publications · 1.3K citations

    18

    h-index

  5. 6

    h-index

1–5