Published 1986
| Version v1
Book
Nuclear reactions in strongly evolved stars
Creators
Description
The mechanism of nuclear reactions, proceeding in strongly evolved stars, is discussed. Laboratory methods of the determination of nuclear reaction rates, which are of importance for helium, carbon, neon, oxygen and silicon burning, are considered. Experimental data are compared with calculations on nuclear reaction models
Additional details
Additional titles
- Original title (Russian)
- Ядерные реакции в сильно проеволюционировавших звездах
Publishing Information
- Publisher
- Mir.
- Imprint Place
- Moscow (USSR)
- Imprint Title
- Nuclear astrophysics
- Journal Page Range
- p. 191-227.
INIS
- Country of Publication
- USSR
- Country of Input or Organization
- USSR
- INIS RN
- 18025587
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CARBON BURNING; CROSS SECTIONS; ENERGY DEPENDENCE; HELIUM BURNING; NEON; NUCLEAR REACTION KINETICS; NUCLEOSYNTHESIS; OXYGEN; SILICON; STARS
- Descriptors DEC
- ELEMENTS; KINETICS; NONMETALS; RARE GASES; REACTION KINETICS; SEMIMETALS; STAR BURNING; SYNTHESIS
Optional Information
- Notes
- Translated from English by Nadezhdin, D.K.; Stel'nitskij, V.S.; Antipova, L.I.; Kopysov, Yu.S.; edited by Masevich, A.G. Imprint:Yadernaya astrofizika.