Spectroscopic Binary Orbits

Spectroscopic Binary Orbits is a computational model in stellar astrophysics that determines the orbital parameters of binary star systems by analyzing periodic Doppler shifts in their spectral lines, distinguishing it from visual or eclipsing binary methods through its reliance on spectroscopic rather than positional or photometric data.

421

Publications

20.8K

Citations

1.1K

Authors

424

Institutions

Publications per year

2017–2026

48

Authors

1.1K

  1. GT
    Guillermo Torres

    Center for Astrophysics Harvard & Smithsonian, United States

    18 publications · 1.9K citations

    17

    h-index

  2. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    19 publications · 1.5K citations

    16

    h-index

  3. SU
    S. Udry

    University of Geneva, Switzerland

    15 publications · 2.1K citations

    14

    h-index

  4. RF
    R. F. Griffin

    University of Cambridge, United Kingdom

    15 publications · 895 citations

    14

    h-index

  5. FC
    Francis C. Fekel

    Tennessee State University, United States

    15 publications · 1.2K citations

    12

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 114 publications · 6.5K citations

    43

    h-index

  2. The Astronomical Journal

    AJ · 99 publications · 4.1K citations

    32

    h-index

  3. Astronomy and Astrophysics

    57 publications · 3.5K citations

    31

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    51 publications · 1.9K citations

    24

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 23 publications · 1.2K citations

    15

    h-index

1–5