activity
20162023
most citedRotation in stellar interiors: General formulation and an asteroseismic-calibrated transport by the Tayler instability

46 citations · 119 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2023★ 46 cited

Rotation in stellar interiors: General formulation and an asteroseismic-calibrated transport by the Tayler instability

P. Eggenberger, F. D. Moyano, J. W. den Hartogh

Context: Asteroseismic measurements of the internal rotation of evolved stars indicate that at least one unknown efficient angular momentum (AM) transport mechanism is needed in st…

astro-ph.SR2022★ 20 cited

Barium stars as tracers of s-process nucleosynthesis in AGB stars II. Using machine learning techniques on 169 stars

J. W. den Hartogh, A. Yagüe López, B. Cseh +7

We aim to analyse the abundance pattern of 169 Barium (Ba) stars, using machine learning techniques and the AGB final surface abundances predicted by Fruity and Monash stellar mode…

astro-ph.GA2021★ 19 cited

Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution

T. C. L. Trueman, B. Côté, A. Yagüe López +5

Analysis of inclusions in primitive meteorites reveals that several short-lived radionuclides (SLRs) with half-lives Myr existed in the early Solar System (ESS). We inves…

astro-ph.SR2021★ 5 cited

First models of s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver

A. Yagüe López, D. A. García-Hernández, P. Ventura +4

Aims. We describe the first s-process post-processing models for asymptotic giant branch (AGB) stars of masses 3, 4 and 5 M at solar metallicity (Z=0.018) computed using the input…

astro-ph.SR2021★ 29 cited

Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System

Hannah E. Brinkman, J. W. den Hartogh, C. L. Doherty +2

Radioactive nuclei were present in the early Solar System, as inferred from analysis of meteorites. Many are produced in massive stars, either during their lives or their final exp…

astro-ph.SR2017

Impacts of nuclear-physics uncertainty in stellar temperatures on the s-process nucleosynthesis

N. Nishimura, G. Cescutti, R. Hirschi +3

We evaluated the uncertainty relevant to s-process nucleosynthesis using a Monte-Carlo centred approach. We are based on a realistic and general prescription of temperature depende…