Binary Compact Objects

Binary Compact Objects is a theoretical construct in astrophysics that refers to a gravitationally bound system consisting of two compact stellar remnants—such as black holes, neutron stars, or white dwarfs—orbiting each other and potentially emitting detectable gravitational waves as they inspiral and merge.

1K

Publications

93.7K

Citations

6.6K

Authors

927

Institutions

Publications per year

2017–2026

481

Variants

Binary Compact Object Systems

Authors

6.6K

  1. RO
    R. O’Shaughnessy

    Rochester Institute of Technology, United States

    33 publications · 11.8K citations

    28

    h-index

  2. NC
    N. Christensen

    Carleton College, United States

    30 publications · 9K citations

    26

    h-index

  3. LB
    Luc Blanchet

    Centre National de la Recherche Scientifique, France

    28 publications · 3.3K citations

    25

    h-index

  4. BS
    B. S. Sathyaprakash

    Cardiff University, United Kingdom

    26 publications · 9.6K citations

    23

    h-index

  5. DB
    D. Brown

    University of Michigan, United States

    28 publications · 13.6K citations

    23

    h-index

1–5 of 6.6K

Venues

  1. The Astrophysical Journal

    ApJ · 174 publications · 17.4K citations

    70

    h-index

  2. 51

    h-index

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

    PRD · 134 publications · 7.7K citations

    50

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    119 publications · 8.3K citations

    47

    h-index

  5. Classical and Quantum Gravity

    56 publications · 7.3K citations

    35

    h-index

1–5