Core Hydrogen Burning

Core Hydrogen Burning is a stellar energy-generation process, belonging to the class of nuclear fusion reactions, in which hydrogen nuclei are fused into helium in the central region of a star under high temperature and pressure, thereby distinguishing it from shell or non-central hydrogen burning phases.

215

Publications

15.5K

Citations

504

Authors

264

Institutions

Publications per year

2017–2026

37

Authors

504

  1. NL
    N. Langer

    University of Bonn, Germany

    15 publications · 2.2K citations

    13

    h-index

  2. UH
    U. Heber

    University of Würzburg, Germany

    8 publications · 688 citations

    8

    h-index

  3. RB
    Richard B. Stothers

    Goddard Institute for Space Studies, United States

    7 publications · 178 citations

    7

    h-index

  4. RG
    R. G. Deupree

    Saint Mary's University, Canada

    6 publications · 220 citations

    6

    h-index

  5. JI
    Jr. Iben Icko

    University of Illinois System, United States

    5 publications · 802 citations

    5

    h-index

1–5 of 504

Venues

  1. The Astrophysical Journal

    ApJ · 77 publications · 5.7K citations

    38

    h-index

  2. Astronomy and Astrophysics

    41 publications · 2.6K citations

    26

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    28 publications · 1.1K citations

    18

    h-index

  4. The Astrophysical Journal Letters

    7 publications · 440 citations

    7

    h-index

  5. The Astronomical Journal

    AJ · 7 publications · 718 citations

    7

    h-index

1–5