Eclipsing Binary Orbits

Eclipsing Binary Orbits 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 regular dips in observed brightness due to mutual eclipses.

375

Publications

16.1K

Citations

1.3K

Authors

477

Institutions

Publications per year

2017–2026

60

Authors

1.3K

  1. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 781 citations

    12

    h-index

  2. TB
    T. Borkovits

    Konkoly Observatory, Hungary

    12 publications · 503 citations

    12

    h-index

  3. AH
    A. H. M. J. Triaud

    University of Geneva, Switzerland

    11 publications · 639 citations

    11

    h-index

  4. GT
    Guillermo Torres

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 731 citations

    11

    h-index

  5. SQ
    S.‐B. Qian

    Chinese Academy of Sciences, China

    10 publications · 339 citations

    10

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 58 publications · 2.7K citations

    30

    h-index

  2. The Astronomical Journal

    AJ · 53 publications · 3.1K citations

    28

    h-index

  3. Astronomy and Astrophysics

    58 publications · 2.6K citations

    27

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    59 publications · 2.1K citations

    26

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 13 publications · 372 citations

    11

    h-index

1–5