Orbital Period Evolution

Orbital Period Evolution is a theoretical construct in binary star dynamics that characterizes the time-varying change in the orbital周期 of a binary system due to mass transfer, angular momentum loss, or gravitational wave radiation, distinguishing it from static orbital models by its intrinsic dependence on evolutionary processes in X-ray binaries.

1.5K

Publications

74.9K

Citations

4.7K

Authors

1.1K

Institutions

Publications per year

2017–2026

361

Authors

4.7K

  1. SQ
    S.‐B. Qian

    Chinese Academy of Sciences, China

    53 publications · 1.7K citations

    24

    h-index

  2. LZ
    Li-Ying Zhu

    Chinese Academy of Sciences, China

    34 publications · 1.2K citations

    21

    h-index

  3. JP
    J. Patterson

    Columbia University, United States

    25 publications · 2.2K citations

    20

    h-index

  4. JH
    J.-J. He

    Chinese Academy of Sciences, China

    28 publications · 1.1K citations

    19

    h-index

  5. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    21 publications · 1K citations

    18

    h-index

1–5 of 4.7K

Venues

  1. The Astrophysical Journal

    ApJ · 305 publications · 22K citations

    73

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    346 publications · 15.5K citations

    61

    h-index

  3. The Astronomical Journal

    AJ · 168 publications · 6.2K citations

    45

    h-index

  4. Astronomy and Astrophysics

    163 publications · 6.2K citations

    41

    h-index

  5. The Astrophysical Journal Letters

    44 publications · 2.6K citations

    31

    h-index

1–5