This paper summarizes our present understanding of the nucleosynthesis and energy
generation in the carbon-nitrogen-oxygen (CNO) cycles and the influence and …

Classical novae are dramatic stellar explosions with an energy release that is only
overcome by supernovae and gamma-ray bursts. These unique cataclysmic events …

The slow neutron capture process in massive stars (weak s process) produces most of the s-
process isotopes between iron and strontium. Neutrons are provided by the 22 Ne (α, n) 25 …

Numerical values of charged-particle thermonuclear reaction rates for nuclei in the A= 14 to
40 region are tabulated. The results are obtained using a method, based on Monte Carlo …

We present nucleosynthesis calculations and the resulting 19 F stellar yields for a large set
of models with different masses and metallicity. During the asymptotic giant branch (AGB) …

The nuclear physics input used to compute the Monte Carlo reaction rates and probability
density functions that are tabulated in the second paper of this series (Paper II) is presented …

New experimental methods and techniques, combined with the development of new
theoretical tools, have opened new avenues to explore nuclear reactions of significance for …

Abstract Knowledge of the astrophysical rate of the 18 F (p, α) 15 O reaction is important for
understanding the γ-ray emission expected from novae and heavy-element production in x …

Classical novae are fascinating stellar explosions at the crossroads of stellar astrophysics,
nuclear physics, and cosmochemistry. In this review, we briefly summarize 30 years of …

Isobaric multiplets can be used to provide reliable mass predictions through the Isobaric
Multiplet Mass Equation (IMME). Isobaric Analogue States (IAS) for isospin multiplets from …