Competitive Accretion

Competitive Accretion is a theoretical model of clustered star formation in which protostars of varying initial masses differentially accrete surrounding gas due to gravitational interactions within a common reservoir, leading to the growth of more massive stars at the expense of their less massive neighbors.

39

Publications

6.2K

Citations

87

Authors

67

Institutions

Publications per year

2017–2026

6

Authors

87

  1. MR
    Matthew R. Bate

    University of Exeter, United Kingdom

    6 publications · 1.7K citations

    6

    h-index

  2. CJ
    C. J. Clarke

    University of Cambridge, United Kingdom

    4 publications · 1.3K citations

    4

    h-index

  3. IA
    I. A. Bonnell

    University of St Andrews, United Kingdom

    4 publications · 1.6K citations

    4

    h-index

  4. JE
    J. E. Pringle

    Institute of Astronomy, Russia

    3 publications · 1.2K citations

    3

    h-index

  5. CF
    Christopher F. McKee

    University of California, Berkeley, United States

    3 publications · 343 citations

    3

    h-index

1–5 of 87

Venues

  1. Monthly Notices of the Royal Astronomical Society

    18 publications · 3.1K citations

    18

    h-index

  2. The Astrophysical Journal

    ApJ · 12 publications · 1.2K citations

    11

    h-index

  3. Astronomy and Astrophysics

    2 publications · 60 citations

    2

    h-index

  4. CERN Document Server (European Organization for Nuclear Research)

    Repository · 1 publications · 221 citations

    1

    h-index

  5. Nature

    1 publications · 163 citations

    1

    h-index

1–5