activity
20192026
most citedSolar oxygen abundance

94 citations · 197 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

Non-LTE corrections for determinations of europium abundances in F-G-K stars in a broad metallicity range

L. I. Mashonkina, S. A. Yakovleva

Europium plays a key role in studies of nucleosynthesis in the rapid (r-) process of neutron capture nuclear reactions and the evolution of the r-process element abundances in gala…

astro-ph.SR202418 cited

3D NLTE modelling of Y and Eu. Centre-to-limb variation and solar abundances

N. Storm, P. S. Barklem, S. A. Yakovleva +6

Context. Abundances of s- and r-process elements in Sun-like stars constrain nucleosynthesis in extreme astrophysical events, such as compact binary mergers and explosions of highl…

astro-ph.SR2023

Theoretical Study of Inelastic Processes in Collisions of Y and Y with Hydrogen Atom

Yu Wang, Sofya Alexeeva, Feng Wang +6

Utilizing a simplified quantum model approach, the low-energy inelastic collision processes between yttrium atoms (ions) and hydrogen atoms have been studied. Rate coefficients cor…

astro-ph.SR202194 cited

Solar oxygen abundance

Maria Bergemann, Richard Hoppe, Ekaterina Semenova +10

Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of the solar photospheric oxygen (O) abundance. New atomic models of O and Ni are use…

astro-ph.SR202020 cited

Influence of Collisions with Hydrogen on Titanium Abundance Determinations in Cool Stars

T. M. Sitnova, S. A. Yakovleva, A. K. Belyaev +1

We performed the non-local thermodynamic equilibrium (non-LTE) calculations for Ti I-II with the updated model atom that includes quantum-mechanical rate coefficients for inelastic…

astro-ph.SR201965 cited

Observational constraints on the origin of the elements II. 3D non-LTE formation of Ba ii lines in the solar atmosphere

A. J. Gallagher, M. Bergemann, R. Collet +5

Context. The pursuit of more realistic spectroscopic modelling and consistent abundances has led us to begin a new series of papers designed to improve current solar and stellar ab…