Search Publications

Abundances of α-Process Elements in Thin-Disk, Thick-Disk, and Halo Stars of the Galaxy: Non-LTE Analysis
DOI: 10.1134/S1063772919090063 Bibcode: 2019ARep...63..726M

Sitnova, T. M.; Mashonkina, L. I.; Pakhomov, Yu. V. +1 more

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 modeling of lines without assuming LTE (non-LTE modeling). A sample of stars with homogeneous data on the abundances of α-process elements has thus been increased to 94. It is shown that appl…

2019 Astronomy Reports
Gaia 16
Flow Structure in the Eclipsing Polar V808 Aur. Results of 3D Numerical Simulations
DOI: 10.1134/S1063772919090087 Bibcode: 2019ARep...63..751Z

Bisikalo, D. V.; Zhilkin, A. G.; Gabdeev, M. M. +1 more

The structure of the flows in the eclipsing polar V808 Aur is studied. Comparison of computations with observed light curves is used to identify and clarify a number of features in the system, such as the drift of the hot spot—the place where the stream from the inner Lagrange point approaches the surface of the white dwarf, changes in the brightn…

2019 Astronomy Reports
Gaia 14
Kinetic Monte Carlo Model for the Precipitation of High-Energy Protons and Hydrogen Atoms into the Atmosphere of Mars with Taking into Account the Measured Magnetic Field
DOI: 10.1134/S1063772919100056 Bibcode: 2019ARep...63..835S

Gérard, J. -C.; Hubert, B.; Shematovich, V. I. +1 more

Results of model computations of the interaction of the high-energy protons and hydrogen atoms (H/H+) precipitating into the Martian atmosphere are presented. These computations were performed using a modification of the kinetic Monte Carlo model developed earlier for the analysis of the data from the MEX/ASPERA-3 instrument onboard the…

2019 Astronomy Reports
MEx 13
Possible Electromagnetic Manifestations of Merging Black Holes
DOI: 10.1134/S1063772919010025 Bibcode: 2019ARep...63....1B

Bisikalo, D. V.; Zhilkin, A. G.; Kurbatov, E. P.

The scenario of a merger of two black holes surrounded by an accretion disk is considered. As a result of the emission of gravitational waves, the mass of the central object decreases, and the accretion disk is perturbed. Computational results show that the main consequence of this perturbation is the formation of a shock propagating from the cent…

2019 Astronomy Reports
INTEGRAL 5
Results of Many-year Photometry of the Herbig Ae Star AB Aur in the Near Infrared
DOI: 10.1134/S1063772919120060 Bibcode: 2019ARep...63.1035S

Grinin, V. P.; Shenavrin, V. I.; Baluev, R. V. +1 more

The results of many-year infrared observations of the Herbig AeBe star AB Aur at 1-5 µm (JHKLM bands) are presented. The duration of the photometric series, together with observations published earlier, is about 18 years. The observations demonstrate that, in contrast to the optical, the star is quite active in the studied infrared range. Th…

2019 Astronomy Reports
Gaia 4
Chemical Composition of Globular Clusters of Milky Way Subsystems from Gaia DR2 Data
DOI: 10.1134/S1063772919120023 Bibcode: 2019ARep...63..998B

Bobylev, V. V.; Bajkova, A. T.; Korchagin, V. I. +1 more

Results of a study of the kinematic and chemical properties of globular clusters of the Milky Way based on data from the Gaia DR2 catalog and meaurements with the Hubble Space Telescope are presented. A new method for dividing globular clusters into Galatic subsystems based on the elements of their Galactic orbits is proposed. Samples of globular …

2019 Astronomy Reports
Gaia eHST 4
V404 CYG/GS 2023+338: Monitoring in the Optical with Robotic Telescopes of the MASTER Global Network during the 2015 Superburst
DOI: 10.1134/S1063772919070059 Bibcode: 2019ARep...63..534L

Rebolo, R.; Buckley, D. A. H.; Giovannelli, F. +23 more

2070 unique, homogeneous photometric and polarization observations of the microquasar in a binary system with a black hole V404 Cyg/GS2023+338 obtained in 2015 with the MASTER global network of robotic telescopes (16 robotic telescopes located at eight points on the Earth in Russia, Spain, South Africa, and Argentina) are presented. MASTER was the…

2019 Astronomy Reports
INTEGRAL 2
Features of the Residual Velocity Ellipsoid of Hot Subdwarfs from the Gaia DR2 Catalog
DOI: 10.1134/S1063772919110027 Bibcode: 2019ARep...63..932B

Bobylev, V. V.; Bajkova, A. T.

The evolution of the parameters of the residual velocity ellipsoid of hot subdwarfs (HSDs) with their position relative to the Galactic plane is traced, using the HSDs selected by Geier et al. from the Gaia DR2 catalog. Parameters of the Galactic rotation are determined for two ∣ z∣ zones. These are used to estimate the gradient of the circular ro…

2019 Astronomy Reports
Gaia 1
Influence of Digital Noise on Interpretation of a Transit Light Curve
DOI: 10.1134/S106377291902001X Bibcode: 2019ARep...63..107A

Abubekerov, M. K.; Gostev, N. Yu.

The algorithms often used for the interpretation of light curves, such as the frequently applied JKTEBOP algorithm, have limited accuracy, which causes rounding errors, and hence a non-physical contribution to the residuals (digital noise). The transit light curve of the binary HD 209458 is used as an example to demonstrate the need to take into a…

2019 Astronomy Reports
eHST 1
Spectroscopy of Globular Clusters in the Spheroidal Dwarf Galaxy IKN
DOI: 10.1134/S1063772919070084 Bibcode: 2019ARep...63..687S

Sharina, M. E.; Shimansky, V. V.

Moderate resolution spectra of four globular clusters in the dwarf spheroidal galaxy IKN obtained with the 6-m telescope of the Special Astrophysical Observatory have been used to determine the radial velocities, ages, and metallicities of the clusters, and also to derive the first approximate estimates of the abundances of Mg, Ca, and C. Cross-co…

2019 Astronomy Reports
eHST 1