Massive Star Structure

Massive Star Structure is a theoretical framework in astrophysics that specifically models the internal composition, energy transport, and evolutionary dynamics of stars with masses significantly exceeding that of the Sun, distinguishing it from general stellar structure theories by focusing on the unique physical processes such as radiation pressure dominance, strong stellar winds, and convective core burning prevalent in high-mass regimes.

290

Publications

20.9K

Citations

972

Authors

464

Institutions

Publications per year

2017–2026

69

Authors

972

  1. SS
    S. Simón‐Díaz

    Instituto de Astrofísica de Canarias, Spain

    13 publications · 969 citations

    13

    h-index

  2. AH
    A. Herrero

    Instituto de Astrofísica de Canarias, Spain

    9 publications · 725 citations

    9

    h-index

  3. QZ
    Qizhou Zhang

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 327 citations

    6

    h-index

  4. NL
    N. Langer

    University of Bonn, Germany

    5 publications · 1.1K citations

    5

    h-index

  5. RC
    R. Cesaroni

    Arcetri Astrophysical Observatory, Italy

    4 publications · 178 citations

    5

    h-index

1–5 of 972

Venues

  1. The Astrophysical Journal

    ApJ · 68 publications · 7.7K citations

    41

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    34 publications · 2.8K citations

    27

    h-index

  3. Astronomy and Astrophysics

    38 publications · 2.5K citations

    24

    h-index

  4. The Astronomical Journal

    AJ · 11 publications · 486 citations

    11

    h-index

  5. Nature

    8 publications · 1K citations

    8

    h-index

1–5