Binary Star Spectroscopy

Binary Star Spectroscopy is a specialized method within stellar spectroscopy that analyzes periodic Doppler shifts in the spectral lines of a star system to detect and characterize the orbital motion and physical properties of two gravitationally bound stars.

975

Publications

48K

Citations

3K

Authors

788

Institutions

Publications per year

2017–2026

124

Authors

3K

  1. CA
    C. Aerts

    KU Leuven, Belgium

    40 publications · 1.8K citations

    27

    h-index

  2. DR
    Douglas R. Gies

    Georgia State University, United States

    30 publications · 1.1K citations

    19

    h-index

  3. KU
    K. Uytterhoeven

    KU Leuven, Belgium

    21 publications · 857 citations

    18

    h-index

  4. MB
    M. Briquet

    KU Leuven, Belgium

    21 publications · 938 citations

    17

    h-index

  5. AF
    A. F. J. Moffat

    Université de Montréal, Canada

    18 publications · 796 citations

    16

    h-index

1–5 of 3K

Venues

  1. The Astrophysical Journal

    ApJ · 192 publications · 11.4K citations

    55

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    186 publications · 9.4K citations

    50

    h-index

  3. Astronomy and Astrophysics

    193 publications · 8.9K citations

    46

    h-index

  4. The Astronomical Journal

    AJ · 117 publications · 5K citations

    37

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 59 publications · 2.5K citations

    25

    h-index

1–5