Pre-main-sequence Binaries

Pre-Main-Sequence Binaries is a binary star system in which both components are pre-main-sequence stars, distinguished from other binary systems by their evolutionary stage prior to the initiation of stable hydrogen fusion in their cores.

277

Publications

14.2K

Citations

787

Authors

346

Institutions

Publications per year

2017–2026

25

Authors

787

  1. JB
    J. Bouvier

    Centre National de la Recherche Scientifique, France

    8 publications · 418 citations

    8

    h-index

  2. RD
    Robert D. Mathieu

    University of Wisconsin–Madison, United States

    7 publications · 965 citations

    7

    h-index

  3. EC
    E. Covino

    Astronomical Observatory of Capodimonte, Italy

    6 publications · 362 citations

    6

    h-index

  4. GM
    G. Micela

    Osservatorio Astronomico di Palermo, Italy

    6 publications · 237 citations

    6

    h-index

  5. MS
    M. Simon

    Stony Brook University, United States

    5 publications · 377 citations

    6

    h-index

1–5 of 787

Venues

  1. The Astrophysical Journal

    ApJ · 66 publications · 4.4K citations

    37

    h-index

  2. Astronomy and Astrophysics

    52 publications · 2.5K citations

    28

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    29 publications · 1.6K citations

    23

    h-index

  4. The Astronomical Journal

    AJ · 29 publications · 1.8K citations

    20

    h-index

  5. Astrophysics and Space Science

    7 publications · 152 citations

    8

    h-index

1–5