activity
20182025
most citedNeutron Star Mergers Might not be the Only Source of r-Process Elements in the Milky Way

248 citations · 564 across the 16 of their papers we have counts for

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Showing 2024Show all

4 papers · 1 filter

astro-ph.SR2024★ 13 cited

Chemical Evolution of R-process Elements in Stars (CERES): IV. An observational run-up of the third r-process peak with Hf, Os, Ir, and Pt

Arthur Alencastro Puls, Jan Kuske, Camilla Juul Hansen +8

The third r-process peak (Os, Ir, Pt) is poorly understood due to observational challenges, with spectral lines located in the blue or near-ultraviolet region of stellar spectra. T…

astro-ph.SR2024★ 4 cited

Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network

Adam Griffiths, Miguel-Á Aloy, Raphael Hirschi +6

Stars with initial mass above roughly 8 solar masses will evolve to form a core made of iron group elements at which point no further exothermic nuclear reactions between charged n…

astro-ph.SR2024★ 2 cited

Do not forget the electrons: Extending moderately-sized nuclear networks for multidimensional hydrodynamic codes

Domingo García-Senz, Rubén M. Cabezón, Moritz Reichert +5

We present here an extended nuclear network, with 90 species, designed for being coupled with hydrodynamic simulations, which includes neutrons, protons, electrons, positrons, and…

astro-ph.HE2024

Nucleosynthesis in magnetorotational supernovae: impact of the magnetic field configuration

M. Reichert, M. Bugli, J. Guilet +3

The production of heavy elements is one of the main by-products of the explosive end of massive stars. A long sought goal is finding differentiated patterns in the nucleosynthesis…