Binary Pulsars

Binary Pulsars is a class of pulsar systems in which a rapidly rotating neutron star is gravitationally bound to a companion star, distinguished from isolated pulsars by the presence of orbital dynamics that enable precision tests of general relativity and the study of mass transfer, gravitational radiation, and relativistic astrophysics.

1.9K

Publications

146K

Citations

5.8K

Authors

1.1K

Institutions

Publications per year

2017–2026

433

Authors

5.8K

  1. MK
    M. Krämer

    University of Manchester, United Kingdom

    127 publications · 18.2K citations

    62

    h-index

  2. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    92 publications · 10.7K citations

    54

    h-index

  3. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    78 publications · 10.2K citations

    53

    h-index

  4. FC
    F. Camilo

    Columbia University, United States

    83 publications · 11.3K citations

    52

    h-index

  5. PC
    P. C. C. Freire

    Max Planck Institute for Radio Astronomy, Germany

    86 publications · 14.2K citations

    50

    h-index

1–5 of 5.8K

Venues

  1. The Astrophysical Journal

    ApJ · 591 publications · 50.5K citations

    112

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    359 publications · 21.4K citations

    72

    h-index

  3. Nature

    102 publications · 12.3K citations

    50

    h-index

  4. Astronomy and Astrophysics

    98 publications · 4.8K citations

    38

    h-index

  5. The Astrophysical Journal Letters

    50 publications · 3K citations

    32

    h-index

1–5