Main-sequence Structure

Main-Sequence Structure is a theoretical astrophysical model that characterizes the internal physical and compositional organization of stars in hydrostatic equilibrium during the phase of core hydrogen fusion, distinguished from other stellar models by its reliance on mass-dependent relationships between temperature, pressure, luminosity, and energy transport mechanisms governing stellar stability and evolution.

210

Publications

14.6K

Citations

616

Authors

282

Institutions

Publications per year

2017–2026

34

Authors

616

  1. GP
    G. Piotto

    Osservatorio Astronomico di Padova, Italy

    10 publications · 1.9K citations

    10

    h-index

  2. LR
    L. R. Bedin

    Osservatorio Astronomico di Padova, Italy

    9 publications · 1.8K citations

    9

    h-index

  3. JA
    Jay Anderson

    Space Telescope Science Institute, United States

    9 publications · 1.8K citations

    9

    h-index

  4. AP
    A. P. Milone

    Osservatorio Astronomico di Padova, Italy

    9 publications · 835 citations

    9

    h-index

  5. SC
    S. Cassisi

    Collurania Teramo Observatory, Italy

    6 publications · 878 citations

    6

    h-index

1–5 of 616

Venues

  1. The Astrophysical Journal

    ApJ · 61 publications · 5.1K citations

    32

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    30 publications · 2.1K citations

    21

    h-index

  3. The Astronomical Journal

    AJ · 27 publications · 1.5K citations

    19

    h-index

  4. Astronomy and Astrophysics

    20 publications · 1.3K citations

    18

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 9 publications · 236 citations

    9

    h-index

1–5