Shell Burning

Shell Burning is a nuclear fusion process in stellar interiors wherein fusion reactions occur in a concentric layer surrounding a degenerate core, distinguished from core burning by its spatial confinement to a shell-like region where temperature and pressure conditions enable the ignition of heavier elements.

101

Publications

6.6K

Citations

264

Authors

169

Institutions

Publications per year

2017–2026

27

Authors

264

  1. MY
    Masayuki Y. Fujimoto

    Hokkaido University, Japan

    4 publications · 621 citations

    4

    h-index

  2. IH
    Izumi Hachisu

    The University of Tokyo, Japan

    3 publications · 314 citations

    4

    h-index

  3. BM
    Bernhard Müller

    Monash University, Australia

    4 publications · 361 citations

    4

    h-index

  4. NL
    N. Langer

    University of Bonn, Germany

    4 publications · 107 citations

    4

    h-index

  5. MF
    M. F. El Eid

    American University of Beirut, Lebanon

    3 publications · 130 citations

    3

    h-index

1–5 of 264

Venues

  1. The Astrophysical Journal

    ApJ · 43 publications · 3.1K citations

    30

    h-index

  2. 12

    h-index

  3. Astronomy and Astrophysics

    5 publications · 158 citations

    5

    h-index

  4. Publications of the Astronomical Society of the Pacific

    PASP · 4 publications · 389 citations

    4

    h-index

  5. The Astrophysical Journal Letters

    3 publications · 69 citations

    3

    h-index

1–5