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 …

The quest to comprehend how nuclear processes influence astrophysical phenomena is
driving experimental and theoretical research programs worldwide. One of the main goals in …

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 …

Nuclear astrophysics is a field at the intersection of nuclear physics and astrophysics, which
seeks to understand the nuclear engines of astronomical objects and the origin of the …

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 …

The radioisotope 26 Al is a key observable for nucleosynthesis in the Galaxy and the
environment of the early Solar System. To properly interpret the large variety of astronomical …

Type I X-ray bursts are violent stellar events that take place in the H/He-rich envelopes of
accreting neutron stars. We have investigated the role played by uncertainties in nuclear …

Proton captures on Mg isotopes play an important role in the Mg–Al cycle active in stellar H-
burning regions. In particular, low-energy nuclear resonances in the 25 Mg (p, γ) 26 Al …

Since 1999, the TRIUMF-ISAC facility has been providing rare isotope beams for nuclear
physics experiments. The three pillars of the program are nuclear structure, nuclear …

We present the first direct measurement of an astrophysical reaction using a radioactive
beam of isomeric nuclei. In particular, we have measured the strength of the key 447-keV …