Binary Neutron Stars

Binary Neutron Stars is a astrophysical system consisting of two neutron stars in a close orbital configuration around a common center of mass, distinguished from other binary systems by the extreme density and compactness of both components, enabling unique phenomena such as gravitational wave emission and potential merger into black holes or hypermassive neutron stars.

2K

Publications

184.8K

Citations

10.6K

Authors

1.1K

Institutions

Publications per year

2017–2026

833

Variants

Bns

Authors

10.6K

  1. MS
    Masaru Shibata

    Kyoto University, Japan

    85 publications · 10.3K citations

    56

    h-index

  2. LR
    Luciano Rezzolla

    Goethe University Frankfurt, Germany

    45 publications · 6.4K citations

    36

    h-index

  3. TD
    Tim Dietrich

    Max Planck Institute for Gravitational Physics, Germany

    43 publications · 9.8K citations

    34

    h-index

  4. KT
    Keisuke Taniguchi

    The University of Tokyo, Japan

    35 publications · 5.3K citations

    33

    h-index

  5. CM
    C. Messenger

    University of Glasgow, United Kingdom

    36 publications · 22.1K citations

    33

    h-index

1–5 of 10.6K

Venues

  1. The Astrophysical Journal

    ApJ · 428 publications · 38.8K citations

    103

    h-index

  2. 86

    h-index

  3. Physical review. D/Physical review. D.

    PRD · 249 publications · 15.8K citations

    70

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    236 publications · 15.6K citations

    69

    h-index

  5. Physical Review Letters

    PRL · 71 publications · 22.3K citations

    50

    h-index

1–5