activity
20042026
most citedThe 12C(a,g)16O reaction and its implications for stellar helium burning

255 citations · 1.8k across the 69 of their papers we have counts for

collaborators
Showing 2019Show all

13 papers · 1 filter

astro-ph.HE201933 cited

The Nucleosynthetic Yields of Core-Collapse Supernovae, prospects for the Next Generation of Gamma-Ray Astronomy

Sydney Andrews, Chris L. Fryer, Samuel W. Jones +2

Though the neutrino-driven convection model for the core-collapse explosion mechanism has received strong support in recent years, there are still many uncertainties in the explosi…

astro-ph.GA2019

The Impact of Nuclear Physics Uncertainties on Galactic Chemical Evolution Predictions

Benoit Côté, Pavel Denissenkov, Falk Herwig +7

Modeling the evolution of the elements in the Milky Way is a multidisciplinary and challenging task. In addition to simulating the 13 billion years evolution of our Galaxy, chemica…

nucl-ex20197 cited

A direct measurement of the 17O(a,g)21Ne reaction in inverse kinematics and its impact on heavy element production

M. P. Taggart, C. Akers, A. M. Laird +33

During the slow neutron capture process in massive stars, reactions on light elements can both produce and absorb neutrons thereby influencing the final heavy element abundances. A…

astro-ph.SR2019

The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints

J. W. den Hartogh, R. Hirschi, M. Lugaro +5

Aims. We investigate the s-process during the AGB phase of stellar models whose cores are enforced to rotate at rates consistent with asteroseismology observations of their progeni…

astro-ph.GA2019

Using failed supernovae to constrain the Galactic r-process element production

B. Wehmeyer, C. Frohlich, B. Côté +2

Rapid neutron capture process (r-process) elements have been detected in a large fraction of metal-poor halo stars, with abundances relative to iron (Fe) that vary by over two orde…

astro-ph.GA2019

Enrichment of the Galactic disc with neutron-capture elements: Mo and Ru

Tamara Mishenina, Marco Pignatari, Tatiana Gorbaneva +4

We present new observational data for the heavy elements molybdenum (Mo, Z = 42) and ruthenium (Ru, Z = 44) in F-, G-, and K-stars belonging to different substructures of the Milky…