Eclipsing Binary Systems

Eclipsing Binary Systems is a subclass of binary star systems in which the orbital plane is oriented such that, from the perspective of the observer, one star periodically passes in front of the other, causing measurable dips in the system’s light curve due to mutual eclipses.

983

Publications

45.5K

Citations

2.5K

Authors

723

Institutions

Publications per year

2017–2026

155

Authors

2.5K

  1. TB
    T. Borkovits

    Konkoly Observatory, Hungary

    22 publications · 803 citations

    19

    h-index

  2. GT
    Guillermo Torres

    Center for Astrophysics Harvard & Smithsonian, United States

    23 publications · 1.8K citations

    19

    h-index

  3. JS
    J. Southworth

    Keele University, United Kingdom

    22 publications · 1.6K citations

    18

    h-index

  4. JV
    J. V. Clausen

    University of Copenhagen, Denmark

    18 publications · 660 citations

    17

    h-index

  5. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    16 publications · 1.3K citations

    16

    h-index

1–5 of 2.5K

Venues

  1. The Astrophysical Journal

    ApJ · 166 publications · 12.8K citations

    52

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    174 publications · 6.7K citations

    43

    h-index

  3. The Astronomical Journal

    AJ · 134 publications · 7.3K citations

    38

    h-index

  4. Astronomy and Astrophysics

    138 publications · 4.7K citations

    36

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  5. Astrophysics and Space Science

    57 publications · 1.8K citations

    22

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1–5