Published January 24, 2008 | Version v1
Journal article

Recent Applications of the THM to the AGB Star Nucleosynthesis

  • 1. Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud and Universita degli Studi di Catania, Catania (Italy)
  • 2. Cyclotron Institute, Texas A and M University, College Station, TX 77843 (United States)

Description

The THM has been applied to the study of reactions involved in the fluorine production in AGB stars with the aim of extending these measurements down to the Gamow peak. Fluorine abundance is important since it allows to constrain mixing models from the comparison of the observed fluorine abundances with the ones predicted by models. In particular the study focuses on the 15N(p,α)12C and the 18O(p,α)15N reactions which can influence fluorine yield as they are part of 19F production (and destruction) network

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
972
Journal Issue
1
Journal Page Range
p. 485-489
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Carpathian summer school of physics 2007 on exotic nuclei and nuclear/particle astrophysics (II)
Dates
21-31 Aug 2007
Place
Sinaia (Romania)

Optional Information

Notes
(c) 2008 American Institute of Physics