Binary Orbital Modulation

Binary Orbital Modulation is a periodic variation in the observed X-ray emission from a compact object in a binary system, arising from the orbital motion that modulates the line-of-sight to the X-ray source through Doppler shifts, eclipse effects, or changes in accretion geometry.

189

Publications

8.5K

Citations

799

Authors

326

Institutions

Publications per year

2017–2026

40

Authors

799

  1. HS
    H. Sana

    KU Leuven, Belgium

    7 publications · 430 citations

    7

    h-index

  2. AF
    A. F. J. Moffat

    Université de Montréal, Canada

    7 publications · 372 citations

    7

    h-index

  3. NL
    N. Langer

    University of Bonn, Germany

    6 publications · 393 citations

    6

    h-index

  4. TS
    T. Shenar

    University of Potsdam, Germany

    6 publications · 393 citations

    6

    h-index

  5. AF
    A. F. Lanza

    Osservatorio Astrofisico di Catania, Italy

    6 publications · 504 citations

    6

    h-index

1–5 of 799

Venues

  1. The Astrophysical Journal

    ApJ · 50 publications · 3K citations

    29

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    48 publications · 1.9K citations

    26

    h-index

  3. Astronomy and Astrophysics

    32 publications · 1.4K citations

    22

    h-index

  4. The Astrophysical Journal Letters

    9 publications · 315 citations

    10

    h-index

  5. The Astronomical Journal

    AJ · 6 publications · 182 citations

    6

    h-index

1–5