Binary Star Formation

Binary Star Formation is the subfield of star-formation theory that investigates the physical processes—primarily core or disk fragmentation and, more rarely, dynamical capture—through which two protostars emerge and become gravitationally bound to co-orbit as a binary stellar system from their natal environment.

2.6K

Publications

185.2K

Citations

6.2K

Authors

1.2K

Institutions

Publications per year

2017–2026

718

Authors

6.2K

  1. QZ
    Qizhou Zhang

    Center for Astrophysics Harvard & Smithsonian, United States

    36 publications · 1.9K citations

    26

    h-index

  2. PC
    P. Caselli

    Max Planck Institute for Extraterrestrial Physics, Germany

    28 publications · 1.5K citations

    23

    h-index

  3. CC
    C. Codella

    Arcetri Astrophysical Observatory, Italy

    30 publications · 1.4K citations

    23

    h-index

  4. RC
    R. Cesaroni

    Arcetri Astrophysical Observatory, Italy

    28 publications · 1.4K citations

    22

    h-index

  5. ZH
    Zhanwen Han

    Chinese Academy of Sciences, China

    26 publications · 3.4K citations

    22

    h-index

1–5 of 6.2K

Venues

  1. The Astrophysical Journal

    ApJ · 739 publications · 64.3K citations

    126

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    567 publications · 38.9K citations

    102

    h-index

  3. Astronomy and Astrophysics

    411 publications · 25.2K citations

    91

    h-index

  4. The Astrophysical Journal Letters

    88 publications · 5.3K citations

    44

    h-index

  5. The Astronomical Journal

    AJ · 111 publications · 6.6K citations

    43

    h-index

1–5