output
19962026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2024 · astro-ph.SRShow all

7 papers · 2 filters

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★ 26 cited

Gaia Data Release 3: spectroscopic binary-star orbital solutions. The SB1 processing chain

E. Gosset, Y. Damerdji, T. Morel +7

Gaia is an astrometric space experiment that is measuring positions, proper motions as well as parallaxes for a huge number of stars. It operates a medium-dispersion spectrometer,…

astro-ph.SR2024★ 14 cited

Binary progenitor systems for Type Ic supernovae

Martín Solar, Michał J. Michałowski, Jakub Nadolny +18

Core-collapse supernovae are explosions of massive stars at the end of their evolution. They are responsible for metal production and for halting star formation, having a significa…

astro-ph.SR2024★ 32 cited

Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost

A. Khalatyan, F. Anders, C. Chiappini +14

In this paper, we explore the feasibility of using machine learning regression as a method of extracting basic stellar parameters and line-of-sight extinctions from spectro-photome…

astro-ph.SR2024★ 5 cited

The true nature of HE0057-5959, the most metal-poor Li-rich star

A. Mucciarelli, P. Bonifacio, L. Monaco +2

The Li-rich stars are a class of rare objects with A(Li) higher than that of other stars in the same evolutionary stage. Their origin is still debated and valuable routes are the C…

astro-ph.SR2024★ 2 cited

Neutron-capture elements in a sample of field metal-poor N-rich dwarfs

M Spite, P Bonifacio, E Caffau +1

The aim of this work is to measure the abundances of n-capture elements in a sample of six metal-poor N-rich dwarfs that were formed in globular clusters, and subsequently became u…