Published August 4, 1997 | Version v1
Journal article

Capture reactions in the helium burning of stars

  • 1. Stuttgart Univ. (Germany). Inst. fuer Strahlenphysik
  • 2. Physique Nucleaire Theorique et Physique Mathematique, Universite Libre de Bruxelles, Campus Plaine CP-229, 1050 Brussels (Belgium)
  • 3. Physikalisches Institut, Universitaet Tuebingen, Auf der Morgenstelle 14, 72076 Tuebingen (Germany)
  • 4. Institut fuer Kernphysik, Technische Universitaet Wien, Wiedner Hauptstrasse 8-10, 1040 Wien (Austria)
  • 5. NCSR Demokritos, POB 60228, 153 10 Aghia Paraskevi, Athens (Greece)

Description

In the helium burning stage of stars there is a main sequence of reactions which is responsible for energy production and nucleosynthesis of the light elements 12C and 16O. Moreover some other reaction sequences may occur as for instance 14N(α,γ)18F(β)18O 18O(α,n)21Ne(α,n)24Mg and 18O(α,γ)22Ne(α,n)25Mg and 22Ne(α,γ)26Mg, 15N(α,γ)19F, 13C(α,n)16O. (orig.)

Additional details

Publishing Information

Journal Title
Nuclear Physics. A
Journal Volume
621
Journal Issue
1-2
Journal Page Range
p. 149-152.
ISSN
0375-9474
CODEN
NUPABL

Conference

Title
4. international symposium on nuclear astrophysics - nuclei in the cosmos (NIC-4).
Dates
20-27 Jun 1996.
Place
Notre Dame, IN (United States).