Orbital Separation Distribution

Orbital Separation Distribution is a statistical construct in astrophysics that characterizes the frequency distribution of projected or physical distances between components in binary star systems, distinguishing it from other binary properties by quantifying the likelihood of formation or survival at specific separations.

130

Publications

8.4K

Citations

628

Authors

312

Institutions

Publications per year

2017–2026

41

Authors

628

  1. AT
    Andreï Tokovinin

    Cerro Tololo Inter-American Observatory, Chile

    5 publications · 305 citations

    5

    h-index

  2. BS
    B. Scott Gaudi

    The Ohio State University, United States

    4 publications · 526 citations

    4

    h-index

  3. MJ
    M. Janson

    Max Planck Institute for Astronomy, Germany

    3 publications · 305 citations

    3

    h-index

  4. NS
    Noam Soker

    Technion – Israel Institute of Technology, Israel

    3 publications · 196 citations

    3

    h-index

  5. MK
    M. Kasper

    European Southern Observatory, Germany

    3 publications · 303 citations

    3

    h-index

1–5 of 628

Venues

  1. The Astrophysical Journal

    ApJ · 32 publications · 2.4K citations

    26

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    26 publications · 1.9K citations

    21

    h-index

  3. The Astronomical Journal

    AJ · 21 publications · 1.7K citations

    16

    h-index

  4. Astronomy and Astrophysics

    10 publications · 644 citations

    10

    h-index

  5. Icarus

    5 publications · 357 citations

    5

    h-index

1–5