Zero-age Main Sequence

The "Zero-Age Main Sequence" is a theoretical locus in the Hertzsprung-Russell diagram representing the position of newly formed main-sequence stars that have just initiated hydrogen fusion in their cores and have not yet undergone significant evolutionary changes in structure or composition.

433

Publications

39.7K

Citations

1.2K

Authors

493

Institutions

Publications per year

2017–2026

85

Variants

Zams

Authors

1.2K

  1. GM
    G. Meynet

    University of Geneva, Switzerland

    13 publications · 2.1K citations

    13

    h-index

  2. CG
    C. Georgy

    University of Geneva, Switzerland

    10 publications · 1.8K citations

    10

    h-index

  3. SE
    Sylvia Ekström

    University of Geneva, Switzerland

    9 publications · 1.8K citations

    9

    h-index

  4. LG
    L. G. Althaus

    Universidad Nacional de La Plata, Argentina

    8 publications · 531 citations

    8

    h-index

  5. CD
    Christian D. Ott

    California Institute of Technology, United States

    7 publications · 1.1K citations

    7

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 143 publications · 13.3K citations

    58

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    91 publications · 7.4K citations

    40

    h-index

  3. Astronomy and Astrophysics

    57 publications · 4.7K citations

    35

    h-index

  4. The Astronomical Journal

    AJ · 33 publications · 2.3K citations

    22

    h-index

  5. The Astrophysical Journal Supplement Series

    11 publications · 1.1K citations

    11

    h-index

1–5