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
Variants
Deuterium Fusion
94
Joseph Filippazzo, Emily L. Rice, Jacqueline K. Faherty et al. · The Astrophysical Journal · 2015 · 361 citations · Full text
Natural Sciences, Astronomy, Physics +17
Imaging Extrasolar Giant Planets
Publications of the Astronomical Society of the Pacific · 2016 · 354 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 94
398
4
h-index
3
h-index
3
h-index
3
h-index
3
h-index
1–5 of 398
221

Centre National de la Recherche Scientifique
Paris, France
10 h-index
23 publications
2.2K citations
California Institute of Technology
Pasadena, United States
10 h-index
19 publications
458 citations
Los Alamos National Laboratory
Los Alamos, United States
7 h-index
18 publications
1.6K citations

University of Toronto
Toronto, Canada
7 h-index
14 publications
1.2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
6 h-index
6 publications
1.2K citations

École Normale Supérieure de Lyon
Lyon, France
5 h-index
10 publications
1K citations
University of California, Berkeley
Berkeley, United States
5 h-index
5 publications
935 citations
Université de Montréal
Montreal, Canada
5 h-index
5 publications
235 citations
1–8 of 221
ApJ · 27 publications · 2.7K citations
23
h-index
10 publications · 820 citations
10
h-index
5 publications · 160 citations
5
h-index
5 publications · 168 citations
5
h-index
AJ · 4 publications · 209 citations
4
h-index
1–5