NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (10)

astro-ph.SR2017

Influence of inelastic collisions with hydrogen atoms on the non-LTE modelling of Ca I and Ca II lines in late-type stars

L. Mashonkina, T. Sitnova, A. K. Belyaev

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

astro-ph.IM2017

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

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

astro-ph.SR2014

Refining the asteroseismic model for the young delta Scuti star HD 144277 using HARPS spectroscopy

Konstanze Zwintz, Tatiana Ryabchikova, Patrick Lenz +8

astro-ph.SR2016

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

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

astro-ph.SR2014

The surface magnetic field and chemical abundance distributions of the B2V helium-strong star HD184927

I. Yakunin, G. Wade, D. Bohlender +8

astro-ph.SR2017

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

astro-ph.SR2015

Systematic NLTE study of the -2.6 < [Fe/H] < 0.2 F and G dwarfs in the solar neighbourhood. I. Stellar atmosphere parameters

T. Sitnova, G. Zhao, L. Mashonkina +9

astro-ph.SR2013

Signs of atmospheric inhomogeneities in cool stars from 1D-NLTE analysis of iron lines

L. Mashonkina, H. -G. Ludwig, A. Korn +2

astro-ph.SR2015

Accuracy of atmospheric parameters of FGK dwarfs determined by spectrum fitting

T. Ryabchikova, N. Piskunov, Yu. Pakhomov +6