Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-04-29
Astronomy and Astrophysics
Astrophysics
13 pages, 13 figures, Latex, accepted for publication in Astronomy and Astrophysics main journal. Also available at http://a
Scientific paper
The abundances of the isotopes of the elements from C to Al produced by the non-explosive CNO, NeNa and MgAl modes of hydrogen burning, as well as by helium burning, are calculated with the thermonuclear rates recommended by the European compilation of reaction rates for astrophysics (NACRE: details about NACRE may be found at http://astro.ulb.ac.be. This electronic address provides many data of nuclear astrophysics interest and also offers the possibility of generating interactively tables of reaction rates for networks and temperature grids selected by the user). The impact of nuclear physics uncertainties on the derived abundances is discussed in the framework of a simple parametric astrophysical model. These calculations have the virtue of being a guide in the selection of the nuclear uncertainties that have to be duly analyzed in detailed model stars, particularly in order to perform meaningful confrontations between abundance observations and predictions. They are also hoped to help nuclear astrophysicists pinpointing the rate uncertainties that have to be reduced most urgently.
Arnould Marcel
Goriely Stephane
Jorissen Alain
No associations
LandOfFree
Non-explosive hydrogen and helium burnings: Abundance predictions from the NACRE reaction rate compilation 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 Non-explosive hydrogen and helium burnings: Abundance predictions from the NACRE reaction rate compilation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-explosive hydrogen and helium burnings: Abundance predictions from the NACRE reaction rate compilation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-679072