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A non-local thermodynamical equilibrium line formation for neutral and singly ionized titanium in model atmospheres of reference A–K stars

Monthly notices of the Royal Astronomical Society, 2016-09, Vol.461 (1), p.1000-1011

2016

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The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis

Astronomy and astrophysics (Berlin), 2017-08, Vol.604

2017

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

Astronomy and astrophysics (Berlin), 2017-09, Vol.605, p.A53

2017

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SYSTEMATIC NON-LTE STUDY OF THE −2.6 ≤ [Fe/H] ≤ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. II. ABUNDANCE PATTERNS FROM Li TO Eu

The Astrophysical journal, 2016-12, Vol.833 (2), p.225

2016

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Detailed abundances of the wide pairs of stars with and without planets: the binary systems 16 Cyg and HD 219542

Monthly notices of the Royal Astronomical Society, 2022-07, Vol.514 (4), p.4958-4968

2022

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

Astronomy and astrophysics (Berlin), 2017-12, Vol.608, p.A89

2017

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Accuracy of atmospheric parameters of FGK dwarfs determined by spectrum fitting

Monthly notices of the Royal Astronomical Society, 2016-02, Vol.456 (2), p.1221-1234

2016

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

Astronomy and astrophysics (Berlin), 2017-08, Vol.604, p.A129

2017

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SYSTEMATIC Non-LTE STUDY OF THE −2.6 ≤ [Fe/H] ≤ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. I. STELLAR ATMOSPHERE PARAMETERS

The Astrophysical journal, 2015-08, Vol.808 (2), p.1-17

2015

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Modern Technologies in Diagnosis of Fungal Keratitis (Review)

Sovremennye tekhnologii v medit͡s︡ine, 2023-01, Vol.15 (2), p.73-84

2023

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Reflexive Control of an Adversary in a Naval Battle: A Psychological View of the Problem

Military Thought, 2020-12, Vol.29 (4), p.70-76

I.V. SITNOVA

2020

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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

Monthly notices of the Royal Astronomical Society, 2022-07, Vol.515 (1), p.1510-1523

2022

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Chemical diversity among A–B stars with low rotational velocities: non-LTE abundance analysis

Monthly notices of the Royal Astronomical Society, 2020-12, Vol.499 (3), p.3706-3719

2020

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A NLTE line formation for neutral and singly ionized calcium in model atmospheres of B-F stars

Monthly notices of the Royal Astronomical Society, 2018-07, Vol.477 (3), p.3343-3352

2018

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

Astronomy and astrophysics (Berlin), 2019-11, Vol.631, p.A43

2019

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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

Monthly notices of the Royal Astronomical Society, 2021-04, Vol.504 (1), p.1183-1200

2021

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FORMATION OF SOCIALLY SIGNIFICANT QUALITIES OF PERSONALITY IN THE LIGHT OF PHILOSOPHICAL, SOCIOLOGICAL AND PSYCHO-PEDAGOGICAL CONCEPTS OF DEVELOPMENT AND FORMATION OF PERSONALITY

Научное мнение, 2023-09 (9), p.147-151

Sitnova, Anastasia A.

2023

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1D non-LTE corrections for chemical abundance analyses of very metal-poor stars

Monthly notices of the Royal Astronomical Society, 2023-07, Vol.524 (3), p.3526-3536

2023

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Ultra metal-poor stars: improved atmospheric parameters and NLTE abundances of magnesium and calcium

Monthly notices of the Royal Astronomical Society, 2019-05, Vol.485 (3), p.3527-3543

2019

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

Monthly notices of the Royal Astronomical Society, 2022-01, Vol.509 (3), p.3626-3642

2022

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The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis

Astronomy and astrophysics (Berlin), 2021-06, Vol.650

2021

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Non-LTE abundance analysis of A-B stars with low rotational velocities – II. Do A-B stars with normal abundances exist?

Monthly notices of the Royal Astronomical Society, 2023-10, Vol.526 (3), p.3386-3399

2023

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Impact of the convective mixing-length parameter α on stellar metallicity

Astronomy and astrophysics (Berlin), 2020-03, Vol.635, p.A176

2020

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Evaluation of the Recent Atomic Data for Fe i Lines Based on Solar and Stellar Spectra

Solar physics, 2019-11, Vol.294 (11), p.1-10, Article 156

2019

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The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis

Astronomy and astrophysics (Berlin), 2017-12, Vol.608

2017

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A non-local thermodynamical equilibrium line formation for neutral and singly ionized titanium in model atmospheres of reference A–K stars

The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis

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

SYSTEMATIC NON-LTE STUDY OF THE −2.6 ≤ [Fe/H] ≤ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. II. ABUNDANCE PATTERNS FROM Li TO Eu

Detailed abundances of the wide pairs of stars with and without planets: the binary systems 16 Cyg and HD 219542

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

Accuracy of atmospheric parameters of FGK dwarfs determined by spectrum fitting

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

SYSTEMATIC Non-LTE STUDY OF THE −2.6 ≤ [Fe/H] ≤ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. I. STELLAR ATMOSPHERE PARAMETERS

Modern Technologies in Diagnosis of Fungal Keratitis (Review)

Reflexive Control of an Adversary in a Naval Battle: A Psychological View of the Problem

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

Chemical diversity among A–B stars with low rotational velocities: non-LTE abundance analysis

A NLTE line formation for neutral and singly ionized calcium in model atmospheres of B-F stars

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

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

FORMATION OF SOCIALLY SIGNIFICANT QUALITIES OF PERSONALITY IN THE LIGHT OF PHILOSOPHICAL, SOCIOLOGICAL AND PSYCHO-PEDAGOGICAL CONCEPTS OF DEVELOPMENT AND FORMATION OF PERSONALITY

1D non-LTE corrections for chemical abundance analyses of very metal-poor stars

Ultra metal-poor stars: improved atmospheric parameters and NLTE abundances of magnesium and calcium

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

The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis

Non-LTE abundance analysis of A-B stars with low rotational velocities – II. Do A-B stars with normal abundances exist?

Impact of the convective mixing-length parameter α on stellar metallicity

Evaluation of the Recent Atomic Data for Fe i Lines Based on Solar and Stellar Spectra

The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis

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