期刊： ASTRONOMY REPORTS, 2023; 67 (9)
The catalog of wide binary stars [1], created on the basis of Gaia EDR3 data and including more than a million pairs, was used to analyze Gaia DR3 dat......
期刊： ASTRONOMY REPORTS, 2023; 67 (10)
This work examines the formation and evolution of meteoroid streams formed during collisions of near-Earth asteroids (NEAs) with objects in the Main A......
期刊： ASTRONOMY REPORTS, 2023; 67 (3)
Clustering of radio pulsars with observable giant pulses (GPs) has been carried out using the principal component analysis. Five parameters were used ......
期刊： ASTRONOMY REPORTS, 2023; 67 (5)
We study the light-time effect in the eclipsing binary system FL Lyr using data of the Kepler and TESS space missions. We demonstrate that the system ......
期刊： ASTRONOMY REPORTS, 2023; 67 (6)
The main aim of this paper is to investigate numerically the dynamical motion properties of the infinitesimal body under the various types of perturba......
期刊： ASTRONOMY REPORTS, 2023; 67 (7)
The results of a study of the variability of maser emission in OH lines in the 18 cm range in the G10.624-0.385 star formation region from monitoring ......
期刊： ASTRONOMY REPORTS, 2023; 67 (9)
Long-period eclipsing binaries (variables) are a valuable source of data for calculating stellar masses. Such objects have a sufficient amount of both......
期刊： ASTRONOMY REPORTS, 2023; 67 (9)
We review and extend the results of our 2021 paper concerning the problem of tidal evolution of a binary system with a rotating primary component with......
期刊： ASTRONOMY REPORTS, 2023; 67 (10)
This paper presents the result of the search for pulses from the fast radio burst FRB 20220912A with the LPA LPI antenna at a frequency of 111 MHz dur......
期刊： ASTRONOMY REPORTS, 2023; 67 (11)
We study the possibility of determining an orbital eccentricity of a binary star system with an exoplanet from both simulated and observed transit lig......
期刊： ASTRONOMY REPORTS, 2023; 67 (3)
The results of modeling the H alpha absorption spectrum of the atmosphere of the hot Jupiter WASP-52b are presented. The atmosphere was modeled with a......
期刊： ASTRONOMY REPORTS, 2023; 67 (3)
In the development and testing of methods for predicting interplanetary coronal mass ejections (ICMEs), it is important to establish their relationshi......
期刊： ASTRONOMY REPORTS, 2023; 67 (10)
We obtained a unique series of photometric data for more than a hundred years for a rapidly rotat-ing single G5 III-IV giant HD 199178 (V1794 Cyg), be......
期刊： ASTRONOMY REPORTS, 2023; 67 (11)
The objective of this research is to investigate the findings in the perturbed restricted three-body problem involving oblate spheroids as the primary......
期刊： ASTRONOMY REPORTS, 2023; 67 (1)
Problems associated with observations and interpretation of the physical mechanisms underlying the generation of hard electromagnetic radiation from l......
