Deuterium Burning

Deuterium Burning is a nuclear fusion process in which deuterium nuclei combine with protons to form helium-3, releasing energy, that occurs in pre-main-sequence stars when gravitational contraction raises core temperatures and densities to levels sufficient to ignite deuterium fusion, distinguishing it from hydrogen burning by its lower ignition threshold and transient nature during early stellar evolution.

94

Publications

7.6K

Citations

398

Authors

221

Institutions

Publications per year

2017–2026

11

Authors

398

  1. RJ
    Ray Jayawardhana

    University of Toronto, Canada

    4 publications · 250 citations

    4

    h-index

  2. IM
    I. Mazzitelli

    Astronomical Observatory of Rome, Italy

    3 publications · 854 citations

    3

    h-index

  3. MR
    M. R. Zapatero Osorio

    Instituto de Astrofísica de Canarias, Spain

    3 publications · 202 citations

    3

    h-index

  4. AJ
    Adam J. Burgasser

    University of California San Diego, United States

    3 publications · 214 citations

    3

    h-index

  5. IB
    I. Baraffe

    École Normale Supérieure de Lyon, France

    3 publications · 136 citations

    3

    h-index

1–5 of 398

Venues

  1. The Astrophysical Journal

    ApJ · 27 publications · 2.7K citations

    23

    h-index

  2. Astronomy and Astrophysics

    10 publications · 820 citations

    10

    h-index

  3. Journal of Nuclear Materials

    5 publications · 160 citations

    5

    h-index

  4. 5

    h-index

  5. The Astronomical Journal

    AJ · 4 publications · 209 citations

    4

    h-index

1–5