Detached Binary Systems

Detached Binary Systems is a type of binary star system in which the two component stars are sufficiently separated in orbit that neither star fills its Roche lobe, thereby preventing mass transfer between the stars and maintaining independent stellar evolution.

142

Publications

7.1K

Citations

402

Authors

218

Institutions

Publications per year

2017–2026

27

Variants

Detached Binaries

Authors

402

  1. RW
    R. W. Hilditch

    University of St Andrews, United Kingdom

    6 publications · 968 citations

    6

    h-index

  2. SQ
    S.‐B. Qian

    Chinese Academy of Sciences, China

    4 publications · 97 citations

    6

    h-index

  3. XZ
    Xiaobin Zhang

    Chinese Academy of Sciences, China

    4 publications · 106 citations

    4

    h-index

  4. LM
    L. Mahy

    KU Leuven, Belgium

    4 publications · 69 citations

    4

    h-index

  5. MM
    Mario Mateo

    University of Michigan, United States

    3 publications · 90 citations

    3

    h-index

1–5 of 402

Venues

  1. Monthly Notices of the Royal Astronomical Society

    40 publications · 2.5K citations

    24

    h-index

  2. The Astrophysical Journal

    ApJ · 28 publications · 2.2K citations

    22

    h-index

  3. Astronomy and Astrophysics

    20 publications · 587 citations

    18

    h-index

  4. The Astronomical Journal

    AJ · 13 publications · 723 citations

    13

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 70 citations

    4

    h-index

1–5