Binary Stellar Evolution

Binary Stellar Evolution is a theoretical framework in astrophysics that models the coeval development and mutual interactions of two gravitationally bound stars, distinguishing itself from single-star evolution by incorporating mass transfer, tidal forces, and orbital dynamics as fundamental drivers of stellar lifecycle changes.

856

Publications

71.7K

Citations

2.9K

Authors

745

Institutions

Publications per year

2017–2026

348

Authors

2.9K

  1. ZH
    Zhanwen Han

    Chinese Academy of Sciences, China

    25 publications · 3.2K citations

    20

    h-index

  2. NL
    N. Langer

    University of Bonn, Germany

    25 publications · 4.9K citations

    20

    h-index

  3. RG
    R. G. Izzard

    University of Cambridge, United Kingdom

    18 publications · 3.7K citations

    18

    h-index

  4. TM
    Thomas M. Tauris

    Max Planck Institute for Radio Astronomy, Germany

    17 publications · 2K citations

    16

    h-index

  5. KB
    Krzysztof Belczyński

    Nicolaus Copernicus Astronomical Center, Poland

    17 publications · 2.5K citations

    16

    h-index

1–5 of 2.9K

Venues

  1. The Astrophysical Journal

    ApJ · 237 publications · 21.7K citations

    78

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    221 publications · 18.3K citations

    73

    h-index

  3. Astronomy and Astrophysics

    112 publications · 7.1K citations

    47

    h-index

  4. The Astrophysical Journal Letters

    35 publications · 2.5K citations

    26

    h-index

  5. 15

    h-index

1–5