activity
20042022
most citedThe 12C(a,g)16O reaction and its implications for stellar helium burning

255 citations · 1.6k across the 44 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA202218 cited

Chemical Evolution of Fluorine in the Milky Way

Kate A. Womack, Fiorenzo Vincenzo, Brad K. Gibson +5

Fluorine has many different potential sites and channels of production, making narrowing down a dominant site of fluorine production particularly challenging. In this work, we inve…

astro-ph.GA202111 cited

The Fe(n, γ)Fe Cross Section from the Surrogate Ratio Method and Its Effect on the Fe Nucleosynthesis

S. Q. Yan, X. Y. Li, K. Nishio +39

The long-lived Fe (with a half-life of 2.62 Myr) is a crucial diagnostic of active nucleosynthesis in the Milky Way galaxy and in supernovae near the solar system. The neutr…

astro-ph.GA2021

UVES analysis of red giants in the bulge globular cluster NGC 6522

B. Barbuy, E. Cantelli, L. Muniz +10

NGC 6522 is a moderately metal-poor bulge globular cluster ([Fe/H]1.0), and it is a well-studied representative among a number of moderately metal-poor blue horizontal bra…

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…

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…