Pre-main-sequence Evolution

Pre-Main-Sequence Evolution is the phase of stellar evolution wherein a protostar contracts gravitationally and accretes mass prior to reaching the main sequence, distinguished from subsequent evolutionary stages by the absence of sustained hydrogen fusion in its core.

420

Publications

37.4K

Citations

792

Authors

394

Institutions

Publications per year

2017–2026

71

Authors

792

  1. GM
    G. Meynet

    University of Geneva, Switzerland

    19 publications · 1.3K citations

    17

    h-index

  2. PE
    P. Eggenberger

    University of Geneva, Switzerland

    13 publications · 625 citations

    13

    h-index

  3. SE
    Sylvia Ekström

    University of Geneva, Switzerland

    11 publications · 1.1K citations

    12

    h-index

  4. CG
    C. Georgy

    University of Geneva, Switzerland

    11 publications · 887 citations

    11

    h-index

  5. SW
    Steven W. Stahler

    University of California, Berkeley, United States

    8 publications · 1.4K citations

    8

    h-index

1–5 of 792

Venues

  1. The Astrophysical Journal

    ApJ · 117 publications · 11.8K citations

    59

    h-index

  2. Astronomy and Astrophysics

    77 publications · 6.7K citations

    38

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    62 publications · 6.3K citations

    33

    h-index

  4. The Astronomical Journal

    AJ · 20 publications · 1.3K citations

    16

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 13 publications · 1.8K citations

    13

    h-index

1–5