Stellar Structure

Stellar Structure is a subfield of stellar astrophysics that analyzes the internal, typically quasi-static configuration of a star—specified by the radial distribution of mass, pressure, temperature, composition, and energy transport— as determined by hydrostatic equilibrium, the equation of state, and energy generation mechanisms.

44.7K

Publications

3M

Citations

42.7K

Authors

4.1K

Institutions

Publications per year

2017–2026

9K

Authors

42.7K

  1. TC
    Timothy C. Beers

    Michigan State University, United States

    183 publications · 23.5K citations

    80

    h-index

  2. MA
    M. Asplund

    Australian National University, Australia

    177 publications · 19.9K citations

    75

    h-index

  3. NL
    N. Langer

    University of Bonn, Germany

    182 publications · 16.6K citations

    71

    h-index

  4. NC
    N. C. Santos

    Universidade do Porto, Portugal

    202 publications · 17.1K citations

    68

    h-index

  5. SU
    S. Udry

    University of Geneva, Switzerland

    192 publications · 16.1K citations

    65

    h-index

1–5 of 42.7K

Venues

  1. The Astrophysical Journal

    ApJ · 13.2K publications · 986K citations

    335

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    7.3K publications · 458K citations

    240

    h-index

  3. Astronomy and Astrophysics

    6.6K publications · 417.1K citations

    226

    h-index

  4. The Astronomical Journal

    AJ · 2.7K publications · 183.6K citations

    177

    h-index

  5. The Astrophysical Journal Supplement Series

    876 publications · 121.3K citations

    172

    h-index

1–5