Eclipsing Binary Stars

Eclipsing Binary Stars is a subclass of binary star systems in which the orbital plane is oriented such that, from the observer's perspective, one star periodically passes in front of the other, causing a measurable decrease in apparent brightness due to mutual eclipses.

1.2K

Publications

58.5K

Citations

2.8K

Authors

733

Institutions

Publications per year

2017–2026

150

Authors

2.8K

  1. JA
    Jerome A. Orosz

    San Diego State University, United States

    22 publications · 4K citations

    21

    h-index

  2. JS
    J. Southworth

    Keele University, United Kingdom

    26 publications · 2K citations

    21

    h-index

  3. GT
    Guillermo Torres

    Center for Astrophysics Harvard & Smithsonian, United States

    29 publications · 2.9K citations

    21

    h-index

  4. PF
    P. F. L. Maxted

    Keele University, United Kingdom

    20 publications · 1.2K citations

    20

    h-index

  5. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    20 publications · 3.2K citations

    19

    h-index

1–5 of 2.8K

Venues

  1. The Astrophysical Journal

    ApJ · 363 publications · 21.6K citations

    67

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  2. Monthly Notices of the Royal Astronomical Society

    160 publications · 6.8K citations

    45

    h-index

  3. The Astronomical Journal

    AJ · 168 publications · 8.8K citations

    43

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  4. Astronomy and Astrophysics

    136 publications · 6.3K citations

    39

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  5. The Astrophysical Journal Supplement Series

    31 publications · 1.8K citations

    20

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1–5