Contact Binary Systems

A Contact Binary System is a type of close binary star system in which both stellar components share a common outer envelope due to filling their respective Roche lobes, leading to direct mass exchange and thermal coupling between the stars.

538

Publications

26.6K

Citations

1.9K

Authors

639

Institutions

Publications per year

2017–2026

106

Variants

Contact Binaries

Authors

1.9K

  1. SM
    S. M. Ruciński

    University of Toronto, Canada

    22 publications · 1.4K citations

    20

    h-index

  2. LZ
    Li-Ying Zhu

    Chinese Academy of Sciences, China

    23 publications · 687 citations

    17

    h-index

  3. SQ
    S.‐B. Qian

    Chinese Academy of Sciences, China

    29 publications · 774 citations

    16

    h-index

  4. JH
    J.-J. He

    Chinese Academy of Sciences, China

    17 publications · 558 citations

    13

    h-index

  5. RW
    R. W. Hilditch

    University of St Andrews, United Kingdom

    14 publications · 787 citations

    13

    h-index

1–5 of 1.9K

Venues

  1. The Astrophysical Journal

    ApJ · 88 publications · 7.7K citations

    43

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    105 publications · 5.1K citations

    40

    h-index

  3. The Astronomical Journal

    AJ · 91 publications · 3.7K citations

    34

    h-index

  4. Astronomy and Astrophysics

    32 publications · 1.6K citations

    21

    h-index

  5. 14

    h-index

1–5