Accretion In Binary Protostars

Accretion in Binary Protostars is a theoretical framework that describes the process by which mass is gravitationally captured and distributed onto two forming stars in a close binary system, distinguishing it from single-star accretion by incorporating the dynamics of shared circumstellar material and orbital interactions.

297

Publications

21.9K

Citations

768

Authors

401

Institutions

Publications per year

2017–2026

67

Authors

768

  1. LT
    L. Testi

    Arcetri Astrophysical Observatory, Italy

    9 publications · 1.5K citations

    9

    h-index

  2. AN
    A. Natta

    Arcetri Astrophysical Observatory, Italy

    8 publications · 1.2K citations

    8

    h-index

  3. KO
    Kazuyuki Omukai

    Tohoku University, Japan

    7 publications · 1.2K citations

    7

    h-index

  4. CJ
    C. J. Clarke

    University of Cambridge, United Kingdom

    7 publications · 532 citations

    7

    h-index

  5. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 861 citations

    6

    h-index

1–5 of 768

Venues

  1. The Astrophysical Journal

    ApJ · 78 publications · 5.5K citations

    41

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    77 publications · 5.4K citations

    38

    h-index

  3. Astronomy and Astrophysics

    50 publications · 4.2K citations

    36

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 10 publications · 189 citations

    10

    h-index

  5. The Astrophysical Journal Letters

    7 publications · 578 citations

    7

    h-index

1–5