Sofya Alexeeva

most citedSystematic non-LTE study of the

- 2.6 \leq

[Fe/H]

\leq 0.2

F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu

169 citations · 201 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.SR2016★ 169 cited

Systematic non-LTE study of the $- 2.6 \leq$ [Fe/H] $\leq 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu

G. Zhao, L. Mashonkina, H. L. Yan +14

For the first time, we present an extensive study of stars with individual non-local thermodynamic equilibrium (NLTE) abundances for 17 chemical elements from Li to Eu in a sample…

astro-ph.SR2016★ 32 cited

NLTE carbon abundance determination in selected A- and B-type stars and the interpretation of C\ione\ emission lines

S. A. Alexeeva, T. A. Ryabchikova, L. I. Mashonkina

We constructed a comprehensive model atom for C\ione\ -- C\ii\ using the most up-to-date atomic data available and evaluated the non-local thermodynamic equilibrium (NLTE) line for…

Systematic non-LTE study of the −2.6≤ [Fe/H] ≤0.2 F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu

NLTE carbon abundance determination in selected A- and B-type stars and the interpretation of C\ione\ emission lines

Systematic non-LTE study of the $- 2.6 \leq$ [Fe/H] $\leq 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu