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The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem
Published 2019-01-01“…In this paper, the second and the last of the series, we present a sequential algorithm to solve the stellar atmosphere problem that may serve as a paradigm for the solution of more general non-linear and non-local problems. …”
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New Methods in Modeling of Hot Stellar Atmospheres
Published 2013-06-01“…The third aim was to check the applicability of the derived formulae and proposed computation methods to obtain high precision self-consistent results in modeling hot plane-parallel stellar atmospheres. Introducing the dimensionless (reduced) local quantities θ = T/Teff and β = P/P(Teff) it has been shown that for hot convection-free stellar atmospheres the curves log θ versus log β reduce an initial grid of models to simple polynomials and bring forth some general features of the model stellar atmospheres. …”
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THE ABUNDANCES IN THE STELLAR ATMOSPHERES IN THE M13 GLOBULAR CLUSTER
Published 2017-07-01Get full text
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Overstable Convective Modes in a Polytropic Stellar Atmosphere
Published 2023-01-01Get full text
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Stellar Atmospheric Parameters for Cool Dwarfs in Gaia Data Release 3
Published 2024-01-01Get full text
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SELECTIVE EXCITATION OF FE-II IN THE LABORATORY AND LATE-TYPE STELLAR ATMOSPHERES
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The Influence of Chemi-Ionization and Recombination Processes on Spectral Line Shapes in Stellar Atmospheres
Published 2011-12-01“…It has been found that the mentioned chemi-ionization and recombination processes dominate over the concurrent electron-atom and electron-ion ionization and recombination processes in all parts of the considered stellar atmospheres. The obtained results demonstrate the fact that the considered processes must have significant influence on the optical properties of stellar atmospheres. …”
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Collisions of Electrons with Alkali, Alkaline and Complex Atoms Relevant to Solar and Stellar Atmospheres
Published 2022-11-01“…In solar and stellar atmospheres, atomic excitation by impact with electrons plays an important role in the formation of spectral lines. …”
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LOTUS: A (Non-) LTE Optimization Tool for Uniform Derivation of Stellar Atmospheric Parameters
Published 2023-01-01Subjects: Get full text
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A New High-Precision Correction Method of Temperature Distribution in Model Stellar Atmospheres
Published 2013-06-01“…The main features of the temperature correction methods, suggested and used in modeling of plane-parallel stellar atmospheres, are discussed. The main features of the new method are described. …”
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Limb-darkening effect of source stars in gravitational microlensing observations in different filters
Published 2020-11-01Subjects: Get full text
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