Contact Binary Stars

Contact Binary Stars is a type of binary star system in which two stellar components orbit so closely that their outer atmospheres physically interact and share a common envelope, distinguishing it from detached or semi-detached systems by direct mass and energy exchange between the stars.

315

Publications

14.3K

Citations

926

Authors

385

Institutions

Publications per year

2017–2026

72

Variants

Contact Binaries

Authors

926

  1. SM
    S. M. Ruciński

    University of Toronto, Canada

    21 publications · 1.5K citations

    20

    h-index

  2. SQ
    S.‐B. Qian

    Chinese Academy of Sciences, China

    23 publications · 461 citations

    14

    h-index

  3. RW
    R. W. Hilditch

    University of St Andrews, United Kingdom

    13 publications · 755 citations

    13

    h-index

  4. JH
    J.-J. He

    Chinese Academy of Sciences, China

    15 publications · 475 citations

    13

    h-index

  5. LZ
    Li-Ying Zhu

    Chinese Academy of Sciences, China

    15 publications · 398 citations

    11

    h-index

1–5 of 926

Venues

  1. The Astrophysical Journal

    ApJ · 44 publications · 3.2K citations

    31

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    64 publications · 2.9K citations

    28

    h-index

  3. The Astronomical Journal

    AJ · 56 publications · 2.3K citations

    28

    h-index

  4. Astronomy and Astrophysics

    17 publications · 576 citations

    15

    h-index

  5. 12

    h-index

1–5