Red Giant Structure

Red Giant Structure is a theoretical astrophysical model that specifies the stratified internal organization of a red giant star, characterized by a dense degenerate helium core surrounded by a hydrogen-burning shell and an extended convective envelope, distinguishing it from the internal architectures of main-sequence or white dwarf stars.

123

Publications

9.7K

Citations

298

Authors

199

Institutions

Publications per year

2017–2026

35

Authors

298

  1. BM
    B. Mosser

    Laboratoire d’études spatiales et d’instrumentation en astrophysique, France

    20 publications · 3.3K citations

    19

    h-index

  2. DS
    Dennis Stello

    The University of Sydney, Australia

    12 publications · 2.5K citations

    12

    h-index

  3. RA
    R. A. García

    Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France

    10 publications · 2.5K citations

    10

    h-index

  4. SH
    S. Hekker

    Aarhus University, Denmark

    10 publications · 2.4K citations

    10

    h-index

  5. JC
    J. Christensen‐Dalsgaard

    Aarhus University, Denmark

    9 publications · 2.2K citations

    9

    h-index

1–5 of 298

Venues

  1. The Astrophysical Journal

    ApJ · 35 publications · 1.9K citations

    22

    h-index

  2. Astronomy and Astrophysics

    21 publications · 2K citations

    20

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    19 publications · 1.7K citations

    15

    h-index

  4. The Astrophysical Journal Letters

    8 publications · 586 citations

    8

    h-index

  5. arXiv (Cornell University)

    Repository · 4 publications · 186 citations

    4

    h-index

1–5