activity
20172021
most citedThe formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis. II. Early chemical enrichment

76 citations · 90 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202111 cited

The formation of the Milky Way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulum II, and Coma Berenices UFDs

T. M. Sitnova, L. I. Mashonkina, A. M. Tatarnikov +6

We present atmospheric parameters and abundances for chemical elements from carbon to barium in metal-poor stars in Segue 1 (seven stars), Coma Berenices (three stars), and Triangu…

astro-ph.SR2019

Abundances of alpha-Process Elements in Thin-Disk, Thick-Disk, and Halo Stars of the Galaxy: Non-LTE Analysis

Lyudmila Mashonkina, Maria Neretina, Tatyana Sitnova +1

The atmospheric parameters and abundances of Mg, Si, Ca, and Ti have been determined for 20 stars using the Gaia DR2 parallaxes, high-resolution spectra, and the non-local thermody…

astro-ph.SR2018

Chemical composition of metal-poor stars in Coma Berenices ultra-faint dwarf galaxy as a proxy to individual chemical enrichment events

Tatyana Sitnova, Lyudmila Mashonkina, Andrey Tatarnikov +3

We present NLTE abundances and atmospheric parameters for three metal-poor stars ([Fe/H]<-2) in Coma Berenices ultra-faint dwarf galaxy (UFD). The derived results are based on new…

astro-ph.IM20173 cited

Program package for the analysis of high resolution high signal-to-noise stellar spectra

N. Piskunov, T. Ryabchikova, Yu. Pakhomov +4

The program package SME (Spectroscopy Made Easy), designed to perform an analysis of stellar spectra using spectral fitting techniques, was updated due to adding new functions (iso…

astro-ph.SR201776 cited

The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis. II. Early chemical enrichment

L. Mashonkina, P. Jablonka, T. Sitnova +2

We present the non-local thermodynamic equilibrium (NLTE) abundances of up to 10 chemical species in a sample of 59 very metal-poor (VMP, -4 < [Fe/H] < -2) stars in seven dwarf sph…

astro-ph.SR2017

The formation of the Milky Way halo and its dwarf satellites, a NLTE-1D abundance analysis. I. Homogeneous set of atmospheric parameters

L. Mashonkina, P. Jablonka, Yu. Pakhomov +2

We present a homogeneous set of accurate atmospheric parameters for a complete sample of very and extremely metal-poor stars in the dwarf spheroidal galaxies (dSphs) Sculptor, Ursa…