Millisecond Pulsars

Millisecond Pulsar is a type of neutron star that belongs to the class of pulsars and is distinguished by its exceptionally short spin period, typically less than 10 milliseconds, resulting from angular momentum transfer in a binary system through accretion.

1.7K

Publications

127.8K

Citations

6K

Authors

1K

Institutions

Publications per year

2017–2026

432

Variants

Millisecond Pulsar

Authors

6K

  1. MK
    M. Krämer

    University of Manchester, United Kingdom

    100 publications · 11.2K citations

    56

    h-index

  2. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    82 publications · 12.3K citations

    55

    h-index

  3. MB
    M. Bailes

    Swinburne University of Technology, Australia

    88 publications · 8.1K citations

    51

    h-index

  4. FC
    F. Camilo

    Columbia University, United States

    80 publications · 8.7K citations

    51

    h-index

  5. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    69 publications · 9.5K citations

    49

    h-index

1–5 of 6K

Venues

  1. The Astrophysical Journal

    ApJ · 578 publications · 40.2K citations

    106

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    348 publications · 20.6K citations

    74

    h-index

  3. The Astrophysical Journal Letters

    88 publications · 11.3K citations

    42

    h-index

  4. Nature

    79 publications · 11.8K citations

    42

    h-index

  5. Astronomy and Astrophysics

    91 publications · 4.8K citations

    39

    h-index

1–5