Binary Dwarf Planet Systems

Binary Dwarf Planet Systems is a dynamical classification of dwarf planet systems in which two gravitationally bound dwarf planets of comparable mass orbit a common barycenter located in the space between them, distinguishing it from satellite-dominated systems by the mutualism and relative mass equivalence of its components.

26

Publications

835

Citations

290

Authors

175

Institutions

Publications per year

2017–2026

13

Authors

290

  1. GR
    G. Ricker

    Massachusetts Institute of Technology, United States

    2 publications · 92 citations

    2

    h-index

  2. DC
    David Charbonneau

    Center for Astrophysics Harvard & Smithsonian, United States

    2 publications · 92 citations

    2

    h-index

  3. ME
    Mark E. Everett

    California Institute of Technology, United States

    2 publications · 57 citations

    2

    h-index

  4. AS
    Avi Shporer

    Center for Astrophysics Harvard & Smithsonian, United States

    2 publications · 85 citations

    2

    h-index

  5. SR
    S. Reffert

    Heidelberg University, Germany

    2 publications · 55 citations

    2

    h-index

1–5 of 290

Venues

  1. 5

    h-index

  2. The Astronomical Journal

    AJ · 3 publications · 85 citations

    3

    h-index

  3. The Astrophysical Journal Letters

    3 publications · 123 citations

    3

    h-index

  4. Astronomy and Astrophysics

    2 publications · 47 citations

    2

    h-index

  5. The Astrophysical Journal

    ApJ · 2 publications · 64 citations

    2

    h-index

1–5