activity
20132026
most citedObservational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars

145 citations · 465 across the 13 of their papers we have counts for

collaborators

13 papers

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.SR2024★ 18 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.SR2022★ 32 cited

Non-LTE abundances of zinc in different spectral type stars and the Galactic [Zn/Fe] trend based on quantum-mechanical data on inelastic processes in zinc-hydrogen collisions

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

We present a new model atom of Zn I-II based on the most up-to-date photoionisation cross-sections, electron-impact excitation rates, and rate coefficients for the Zn I + H I and Z…

physics.atom-ph2022

Inelastic processes in strontium-hydrogen collisions and their impact on non-LTE calculations

Svetlana A. Yakovleva, Andrey K. Belyaev, Lyudmila I. Mashonkina

Inelastic processes rate coefficients for low-energy Sr + H, Sr + H, Sr + H and Sr + H collisions are calculated using multichannel quantum model approach. 3…

cond-mat.stat-mech2022★ 15 cited

Geometric Upper Critical Dimensions of the Ising Model

Sheng Fang, Zongzheng Zhou, Youjin Deng

The upper critical dimension of the Ising model is known to be , above which critical behavior is regarded as trivial. We hereby argue from extensive simulations that, in th…

astro-ph.SR2021★ 18 cited

The formation of the Milky Way halo and its dwarf satellites: A NLTE-1D abundance analysis. V. The Sextans galaxy

L. Mashonkina, Yu. V. Pakhomov, T. Sitnova +3

We present a homogeneous set of accurate atmospheric parameters for a sample of eleven very metal-poor (-3.32 <= [Fe/H] <= -2.61) stars in the Sextans dwarf spheroidal galaxy (dSph…

astro-ph.SR2021★ 94 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.SR2020★ 20 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.SR2019★ 65 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…

astro-ph.SR2019★ 23 cited

Influence of inelastic collisions with hydrogen atoms on the non-LTE line formation for Fe I and Fe II in the 1D model atmospheres of late-type stars

Lyudmila Mashonkina, Tatyana Sitnova, Svetlana A. Yakovleva +1

Iron plays a crucial role in studies of late-type stars. In their atmospheres, Fe I is the minority species and its lines are subject to the departures from LTE. In contrast, one b…

astro-ph.SR2019★ 145 cited

Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars

Maria Bergemann, Andrew J. Gallagher, Philipp Eitner +9

Manganese (Mn) is a key Fe-group elements, commonly employed in stellar population and nucleosynthesis studies to explore the role of SN Ia. We have developed a new non-local therm…

physics.atom-ph2013★ 35 cited

Charge transfer in the cold Yb + Rb collisions

Elvira R. Sayfutyarova, Alexei A. Buchachenko, Svetlana A. Yakovleva +1

Charge-transfer cold Yb + Rb collision dynamics is investigated theoretically using high-level {\it ab initio} potential energy curves, dipole moment functions and nonadiabatic…