Binary Star Hosts

Binary Star Hosts is a class of exoplanet host systems in which the central gravitational and stellar environment consists of two gravitationally bound stars, distinguishing it from single-star host systems by introducing dynamic interactions that can influence planetary formation, stability, and orbital evolution.

102

Publications

5.7K

Citations

505

Authors

286

Institutions

Publications per year

2017–2026

34

Variants

Binary Exoplanet Host Systems

Authors

505

  1. MM
    M. Mugrauer

    Friedrich Schiller University Jena, Germany

    9 publications · 721 citations

    9

    h-index

  2. RN
    R. Neuhäuser

    Friedrich Schiller University Jena, Germany

    7 publications · 633 citations

    7

    h-index

  3. PF
    P. F. L. Maxted

    Keele University, United Kingdom

    6 publications · 559 citations

    6

    h-index

  4. DQ
    D. Queloz

    University of Geneva, Switzerland

    4 publications · 458 citations

    4

    h-index

  5. AS
    Andreas Seifahrt

    University of Chicago, United States

    4 publications · 397 citations

    4

    h-index

1–5 of 505

Venues

  1. Monthly Notices of the Royal Astronomical Society

    22 publications · 1.1K citations

    18

    h-index

  2. Astronomy and Astrophysics

    19 publications · 989 citations

    17

    h-index

  3. The Astrophysical Journal

    ApJ · 16 publications · 925 citations

    14

    h-index

  4. The Astronomical Journal

    AJ · 10 publications · 623 citations

    10

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 3 publications · 152 citations

    3

    h-index

1–5