Pre-main-sequence Binary Systems

Pre-Main-Sequence Binary Systems is a theoretical construct in stellar astrophysics denoting a class of gravitationally bound binary star systems in which both components are pre-main-sequence stars尚未 having reached hydrostatic equilibrium on the main sequence.

74

Publications

4.4K

Citations

255

Authors

153

Institutions

Publications per year

2017–2026

13

Authors

255

  1. RD
    Robert D. Mathieu

    University of Wisconsin–Madison, United States

    6 publications · 714 citations

    6

    h-index

  2. JB
    J. Bouvier

    Centre National de la Recherche Scientifique, France

    4 publications · 325 citations

    4

    h-index

  3. OC
    O. Chesneau

    Centre National de la Recherche Scientifique, France

    3 publications · 96 citations

    3

    h-index

  4. PG
    P. García

    Universidade do Porto, Portugal

    3 publications · 73 citations

    3

    h-index

  5. MB
    M. Benisty

    Centre National de la Recherche Scientifique, France

    3 publications · 73 citations

    3

    h-index

1–5 of 255

Venues

  1. The Astrophysical Journal

    ApJ · 16 publications · 1.3K citations

    16

    h-index

  2. 13

    h-index

  3. Astronomy and Astrophysics

    15 publications · 569 citations

    12

    h-index

  4. The Astronomical Journal

    AJ · 7 publications · 151 citations

    7

    h-index

  5. arXiv (Cornell University)

    Repository · 2 publications · 38 citations

    2

    h-index

1–5