482 citations · 1.2k across the 6 of their papers we have counts for
6 papers
Chemical Evolution of R-process Elements in Stars (CERES). I. Stellar parameters and chemical abundances from Na to Zr
Linda Lombardo, Piercarlo Bonifacio, Patrick François +10
Aims. The Chemical Evolution of R-process Elements in Stars (CERES) project aims to provide a homogeneous analysis of a sample of metal-poor stars ([Fe/H]<-1.5). We present the ste…
Neutrino-driven winds from neutron star merger remnants
Albino Perego, Stephan Rosswog, Ruben Cabezon +4
We present a detailed, 3D hydrodynamics study of the neutrino-driven winds that emerge from the remnant of a NS merger. Our simulations are performed with the Newtonian, Eulerian c…
Europium production: neutron star mergers versus core-collapse supernovae
F. Matteucci, D. Romano, A. Arcones +2
We have explored the Eu production in the Milky Way by means of a very detailed chemical evolution model. In particular, we have assumed that Eu is formed in merging neutron star (…
The long-term evolution of neutron star merger remnants - I. The impact of r-process nucleosynthesis
S. Rosswog, O. Korobkin, A. Arcones +2
We follow the longterm evolution of the dynamic ejecta of neutron star mergers for up to 100 years and over a density range of roughly 40 orders of magnitude. We include the nuclea…
Nucleosynthesis-relevant conditions in neutrino-driven supernova outflows. II. The reverse shock in two-dimensional simulations
A. Arcones, H. -T. Janka
After the initiation of the explosion of core-collapse supernovae, neutrinos emitted from the nascent neutron star drive a supersonic baryonic outflow. This neutrino-driven wind in…
Production of Light Element Primary Process nuclei in neutrino-driven winds
A. Arcones, F. Montes
We present first comparisons between Light Element Primary Process (LEPP) abundances observed in some ultra metal poor (UMP) stars and nucleosynthesis calculations based on long-ti…