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Article
The Program Magreg for Determining the Longitudinal Component of Stellar Magnetic Fields from Spectropolarimetric Observations
The computer program magreg in IDL language has been developed for determining the longitudinal component Bz of the magnetic field of stars. The program has been tested on observations of a number of objects a...
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Article
Astrophysical Space Mission Astron-2 for an All-Sky Survey in the Ultraviolet Spectral Domain
This paper presents the project of the space astrophysical observatory Astron-2 aimed to carry out the all-sky spectral and photometric survey in the ultraviolet spectral region (115–310 nm). The major instrum...
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Article
Activity of the Star bScl Observed by the TESS Space Telescope
The rotational and flare activity of the chemically peculiar star B9.5IIIpHgMnSi βScl is studied using data from the archive of the TESS space mission. Rotational modulation of the brightness is clearly visibl...
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Article
Activity of the Red Dwarf FR Cnc from Observations with a Robotic IRT-20 Telescope at the Zvenigorod Observatory of INASAN
We present the results of our new photometric observations of the chromospherically active star FR Cnc performed with a robotic telescope at the Zvenigorod Observatory of INASAN in March 2019. The observations...
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Article
Activity of the Star ET Dra
V-band photometric observations of the FK Com type star ET Dra were made at the Zvenigorod observatory (INASAN) during March-April 2018. The new data were used in a solution of the inverse problem of recoverin...
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Article
Areas, Lifetimes, and Magnetic Fields of Starspots
The results of applying a method developed by us for determining the spottedness parameter A to data on the brightness variation of 34030 objects based on observations with the Kepler space telescope are prese...
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Article
Brightness Variability of 12 ROTD A-Stars
The brightness variability of 12 stars of spectral class A which are type ROTD objects is analyzed. The power spectra of these objects contain characteristic features including a amplitude-dominant narrow peak...
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Article
Vertical Chromium Distribution in the Atmospheres of CP Stars. II. Modeling
Vertical chromium distributions in the atmospheres of several Ap and Am stars are fitted using detailed modeling of the profiles of CrII lines. The vertical distributions obtained for Ap stars are consistent w...
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Article
Vertical Chromium Distribution in the Atmosphere of a Chemically Peculiar Star. I. Diagnostics
On the basis of CCD spectrograms obtained with high resolution at the Coudé focus of the 2.6-m telescope of the Crimean Astrophysical Observatory, Cr II lines lying in the wings of the Hβ hydrogen line are inv...
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Article
Superlithium HD9746 – A Brilliant Case of NLTE in Stellar Spectra
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Article
CCD Observations of Comet Hale-Bopp at Shajn Telescope I. Coude spectra
Spectroscopic observations of Comet Hale-Bopp were made at the 2.6 m Shajn Telescope of the Crimean Astrophysical Observatory. Some spectra were obtained with high spectral resolution, FWHM = 0.18–0.4Å, in the...
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Article
The "F str 4077" star HD 177645 as a possible barium dwarf star
The abundances of 12 elements in the atmosphere of the "F str 4077" star HD 177645 have been determined from new spectroscopic observations with the CCD camera and the model atmosphere method. The overabundanc...
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Article
Magnetic fields and the abundance of iron at the surface of late-type dwarfs
A program package developed for implementation of the Stenflo-Lindegren method for investigation of magnetic fields with complex structure is described. It has been used to carry out magnetic field diagnostics...
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Article
Possible presence of magnetic fields and iron content of atmospheres of “Metallic” Am-stars
Measurements with a CCD camera were made of two Fell lines at λ=6747.7 Å and 6149.2 Å in the spectra of 12 Am stars. The greater line strength of Fell λ 6147.7 Å relative to that of λ 6149.2 Å can be taken as .....
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Chapter and Conference Paper
Is ξ Boo AB a young or an evolved system? a model atmosphere analysis
We perform a model atmosphere analysis of ξ Boo A, and make estimates for the secondary component. The abundances of 25 elements for ξ Boo A are obtained with the parameters: T eff=(5300 ± 100) K, log g= 4.1 ± 0....
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Chapter and Conference Paper
Spectroscopic analysis of HR 1099
We have calculated synthetic spectra for HR 1099 for the wavelenffth region λ6425-6445 Å, which includes the CaI λ6439 Å and Fel λ6430 Å lines, often used for the surface imaging of rapidly rotating late-type ...
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Article
Element abundances in the atmosphere of the chemically peculiar star β Cr B
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Article
Determination of the uranium abundance in the Ap star 73 Dra using the line U II λ 3859.58
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Article
Thorium abundance in the atmospheres of Am stars
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Article
The chemical composition of the atmospheres, the masses, radii, and other parameters of four Am stars