Pulsar Winds

Pulsar Winds is a high-energy astrophysical plasma outflow emanating from the magnetosphere of a rotating neutron star, distinguished by its relativistic particle content and strong electromagnetic fields driven by the star's rotational energy loss.

264

Publications

17.1K

Citations

916

Authors

344

Institutions

Publications per year

2017–2026

44

Variants

Pulsar Wind

Authors

916

  1. FA
    F. Aharonian

    Max Planck Institute for Nuclear Physics, Germany

    14 publications · 1K citations

    14

    h-index

  2. DK
    D. Khangulyan

    Max Planck Institute for Nuclear Physics, Germany

    12 publications · 639 citations

    12

    h-index

  3. NB
    N. Bucciantini

    Arcetri Astrophysical Observatory, Italy

    10 publications · 646 citations

    10

    h-index

  4. VB
    V. Bosch-Ramón

    Universitat de Barcelona, Spain

    11 publications · 335 citations

    10

    h-index

  5. EA
    Elena Amato

    Arcetri Astrophysical Observatory, Italy

    9 publications · 545 citations

    9

    h-index

1–5 of 916

Venues

  1. The Astrophysical Journal

    ApJ · 67 publications · 5.2K citations

    39

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    44 publications · 2.9K citations

    29

    h-index

  3. Astronomy and Astrophysics

    41 publications · 2.6K citations

    29

    h-index

  4. arXiv (Cornell University)

    Repository · 8 publications · 190 citations

    8

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 8 publications · 566 citations

    8

    h-index

1–5