Photometric Binaries

Photometric Binaries is a class of binary star systems identified and characterized by periodic variations in their observed brightness, arising from mutual eclipses or distortions in their shapes due to gravitational interaction, detectable through photometric measurements without requiring direct spectral or positional resolution.

619

Publications

28.7K

Citations

2K

Authors

677

Institutions

Publications per year

2017–2026

99

Authors

2K

  1. SQ
    S.‐B. Qian

    Chinese Academy of Sciences, China

    33 publications · 1.1K citations

    21

    h-index

  2. LZ
    Li-Ying Zhu

    Chinese Academy of Sciences, China

    19 publications · 730 citations

    16

    h-index

  3. JH
    J.-J. He

    Chinese Academy of Sciences, China

    20 publications · 730 citations

    16

    h-index

  4. YY
    Yuangui Yang

    Huaibei Normal University, China

    17 publications · 498 citations

    13

    h-index

  5. BS
    Boonrucksar Soonthornthum

    Chinese Academy of Sciences, China

    12 publications · 516 citations

    12

    h-index

1–5 of 2K

Venues

  1. The Astrophysical Journal

    ApJ · 103 publications · 8.3K citations

    43

    h-index

  2. The Astronomical Journal

    AJ · 121 publications · 5.1K citations

    37

    h-index

  3. Astronomy and Astrophysics

    85 publications · 4K citations

    36

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    103 publications · 3.8K citations

    36

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 20 publications · 497 citations

    16

    h-index

1–5