Overcontact Binary Stars

Overcontact Binary Stars is a type of close binary star system in which both component stars fill and share a common outer envelope, resulting in continuous mass transfer and synchronized orbital and rotational motion due to their deeply interacting configurations.

43

Publications

2.8K

Citations

136

Authors

92

Institutions

Publications per year

2017–2026

4

Variants

W Uma StarsW Ursae Majoris Variables

Authors

136

  1. SQ
    S.‐B. Qian

    Chinese Academy of Sciences, China

    15 publications · 721 citations

    14

    h-index

  2. LZ
    Li-Ying Zhu

    Chinese Academy of Sciences, China

    11 publications · 569 citations

    11

    h-index

  3. BS
    Boonrucksar Soonthornthum

    Chinese Academy of Sciences, China

    10 publications · 521 citations

    10

    h-index

  4. JH
    J.-J. He

    Chinese Academy of Sciences, China

    10 publications · 547 citations

    10

    h-index

  5. SQ
    S. Qian

    Chinese Academy of Sciences, China

    6 publications · 354 citations

    6

    h-index

1–5 of 136

Venues

  1. The Astronomical Journal

    AJ · 22 publications · 1.5K citations

    19

    h-index

  2. The Astrophysical Journal

    ApJ · 5 publications · 163 citations

    5

    h-index

  3. Astronomy and Astrophysics

    5 publications · 770 citations

    5

    h-index

  4. 4

    h-index

  5. 3

    h-index

1–5