Binary Orbital Decay

Binary Orbital Decay is a physical phenomenon in astrophysics wherein the orbital separation between two compact objects in a binary star system gradually decreases over time due to the emission of gravitational radiation or mass transfer, leading to an increase in orbital frequency and eventual coalescence.

192

Publications

17.2K

Citations

624

Authors

378

Institutions

Publications per year

2017–2026

72

Authors

624

  1. DL
    Dong Lai

    Cornell University, United States

    13 publications · 616 citations

    13

    h-index

  2. KY
    Kent Yagi

    University of Virginia, United States

    7 publications · 487 citations

    7

    h-index

  3. LM
    Lucio Mayer

    University of Zurich, Switzerland

    6 publications · 423 citations

    6

    h-index

  4. IH
    I. H. Stairs

    University of British Columbia, Canada

    6 publications · 5.2K citations

    6

    h-index

  5. NY
    Nicolás Yunes

    Montana State University, United States

    6 publications · 694 citations

    6

    h-index

1–5 of 624

Venues

  1. Monthly Notices of the Royal Astronomical Society

    47 publications · 3.3K citations

    31

    h-index

  2. The Astrophysical Journal

    ApJ · 42 publications · 3.7K citations

    29

    h-index

  3. The Astrophysical Journal Letters

    15 publications · 874 citations

    14

    h-index

  4. Astronomy and Astrophysics

    11 publications · 564 citations

    11

    h-index

  5. 10

    h-index

1–5