Nucleosynthesis in TP-AGB stars and the production of 19F

Details Nucleosynthesis in TP-AGB stars and the production of 19F Nucleosynthesis in TP-AGB stars and the production of 19F

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718..155g&link_type=abstract

Nuclear Physics A, Volume 718, p. 155-158.

Physics

Nuclear Physics

Scientific paper

Low-energy resonances in the reaction 18O(α,γ) have been measured using a highly efficient γ ray coincidence detector system. These resonances dominate the reaction rate for temperatures typical for TP-AGB stars (0.1-0.3 GK). Preliminary results reduce the reaction rate by up to a factor of three at these temperatures. While this leads to an enhancement of the fluorine production in TP-AGB stars, it is not sufficient to explain the observed fluorine abundances in the surface of red giants.

Affiliated with

Also associated with

No associations

Rating

Nucleosynthesis in TP-AGB stars and the production of 19F does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Nucleosynthesis in TP-AGB stars and the production of 19F, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nucleosynthesis in TP-AGB stars and the production of 19F will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1471506