Pulsar Glitches

Pulsar Glitches is an observed phenomenon in pulsar timing characterized by a sudden increase in rotational frequency followed by a gradual relaxation, distinguishing it from steady spin-down trends and other timing anomalies through its transient and unpredictable nature.

289

Publications

18.2K

Citations

2.2K

Authors

512

Institutions

Publications per year

2017–2026

88

Authors

2.2K

  1. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    28 publications · 2.4K citations

    22

    h-index

  2. VM
    V. M. Kaspi

    McGill University, Canada

    19 publications · 1.7K citations

    18

    h-index

  3. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    20 publications · 1.5K citations

    18

    h-index

  4. BH
    B. Haskell

    Nicolaus Copernicus Astronomical Center, Poland

    18 publications · 872 citations

    16

    h-index

  5. AM
    A. Melatos

    The University of Melbourne, Australia

    20 publications · 1.2K citations

    15

    h-index

1–5 of 2.2K

Venues

  1. The Astrophysical Journal

    ApJ · 73 publications · 5.9K citations

    44

    h-index

  2. 40

    h-index

  3. Physical Review Letters

    PRL · 10 publications · 1.1K citations

    10

    h-index

  4. Astronomy and Astrophysics

    9 publications · 342 citations

    9

    h-index

  5. Nature

    9 publications · 1.2K citations

    9

    h-index

1–5