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Activity of the Young Star with an Exoplanet Kepler-1627
DOI: 10.1134/S1063773722040041 Bibcode: 2022AstL...48..267S

Savanov, I. S.

Based on data from the Kepler Space Telescope archive, we have studied the photometric variability of the young solar analog Kepler-1627, a G8V-type star with a planet of 3.777 Earth radii in size and an orbital period ${∼}$7.2 days. Kepler-1627 is a member of the $δ$ Lyr cluster with an age of 38 Myr and is currently the system with the youngest …

2022 Astronomy Letters
Gaia 2
Kinematics of the Galaxy from Young Open Star Clusters with Data from the Gaia EDR3 Catalogue
DOI: 10.1134/S106377372112001X Bibcode: 2022AstL...48....9B

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

We have analyzed the kinematics of open star clusters (OSCs) with the proper motions and distances calculated by Hao et al. based on Gaia EDR3 data. The mean line-of-sight velocities are known for a number of clusters from this list. We show that the Galactic rotation parameters determined from samples of OSCs with various ages are in good agreeme…

2022 Astronomy Letters
Gaia 2
Estimation of the Mass of the Very Massive Galaxy Cluster SRGe CL2305.2-2248 from Strong Lensing
DOI: 10.1134/S1063773722010042 Bibcode: 2022AstL...48....1K

Bikmaev, I. F.; Gilfanov, M. R.; Khamitov, I. M. +10 more

SRGe CL2305.2-2248 (SPT-CL J2305-2248, ACT-CL J2305.1-2248) is one of the most massive galaxy clusters at high redshifts ($z∼eq 0.76$) and is of great interest for cosmology. Deep images have been obtained at the Russian-Turkish 1.5-m telescope (RTT-150) for an optical identification of this cluster. In combination with the open Hubble Space Teles…

2022 Astronomy Letters
eHST 2
A Three-Dimensional Analytical Model of the Interstellar Extinction within the Nearest Kiloparsec
DOI: 10.1134/S1063773722100024 Bibcode: 2022AstL...48..578G

Savchenko, S. S.; Gontcharov, G. A.; Il'in, V. B. +6 more

We present a new version of our analytical model of the spatial interstellar extinction variations within the nearest kiloparsec from the Sun. This model treats the three-dimensional (3D) dust distribution as a superposition of three overlapping layers: (1) the layer along the Galactic midplane, (2) the layer in the Gould Belt, and (3) the layer p…

2022 Astronomy Letters
Gaia 2
Link between the Optical and Radio Frames from Gaia DR3 Data and VLBI Measurements
DOI: 10.1134/S1063773722110032 Bibcode: 2022AstL...48..790B

Bobylev, V. V.

Based on published data, we have assembled a sample of 126 radio stars with the trigonometric parallaxes and proper motions measured by VLBI and available in the Gaia DR3 catalogue (in fact, Gaia EDR3). Our analysis of the Gaia-VLBI proper motion differences for 84 radio stars based on the model of solid-body mutual rotation has revealed no rotati…

2022 Astronomy Letters
Gaia 2
Study of the X-ray Pulsar IGR J21343+4738 Based on NuSTAR, Swift, and SRG Data
DOI: 10.1134/S106377372211007X Bibcode: 2022AstL...48..798G

Lutovinov, A. A.; Molkov, S. V.; Semena, A. N. +1 more

We present the results of our study of the X-ray pulsar IGR J21343+4738 based on NuSTAR, Swift, and SRG observations in the wide energy range 0.3-79 keV. The absence of absorption features in the energy spectra of the source, both averaged and phase-resolved ones, has allowed us to estimate the upper and lower limits on the magnetic field of the n…

2022 Astronomy Letters
XMM-Newton 2
FG Sge: New Multicolor Photometry and Short-Term Dust Shell Clearing in 2019
DOI: 10.1134/S1063773722060019 Bibcode: 2022AstL...48..329A

Arkhipova, V. P.; Ikonnikova, N. P.; Tatarnikov, A. M. +6 more

We present the results of a new stage of the long-term photometric study of FG Sge which is a quickly evolving central star of the planetary nebula Hen 1-5. Our new observations carried out on the SAI MSU telescopes in the optical ($BVRCIC$) and infrared (IR) ($JHKLM$) regions in 2008-2021 and 2013-2021, respectively, allowed…

2022 Astronomy Letters
Gaia 1
Kinematics of OB Stars with Data from the LAMOST and Gaia Catalogues
DOI: 10.1134/S1063773722040016 Bibcode: 2022AstL...48..243B

Bobylev, V. V.; Bajkova, A. T.; Karelin, G. M.

We have analyzed the kinematics of OB stars from the list by Xiang et al. (2021) that contains ${∼}13 000$ single OB stars. For these stars there are photometric distance estimates and proper motions from the Gaia catalogue and line-of-sight velocities from the LAMOST catalogue. Based on a sample of single OB stars and using the photometric distan…

2022 Astronomy Letters
Gaia 1
Influence of Active Regions on Solar Wind Characteristics at the Cycle Maximum
DOI: 10.1134/S1063773722070039 Bibcode: 2022AstL...48..406B

Reva, A. A.; Kirichenko, A. S.; Ulyanov, A. S. +2 more

Active regions (ARs) on the Sun are discussed as a possible source of the slow solar wind (SW) whose origin is still a subject of debates. In this paper we present experimental evidence for the possible influence of ARs on the SW speed and temperature near the maximum of solar cycle 23 (2000-2002). We have studied separately the characteristics of…

2022 Astronomy Letters
SOHO 1
SRG/eROSITA Survey in the Lockman Hole: Classification of X-ray Sources
DOI: 10.1134/S1063773722110020 Bibcode: 2022AstL...48..755B

Gilfanov, M. R.; Belvedersky, M. I.; Bykov, S. D.

We have classified the X-ray sources detected by the SRG/eROSITA telescope in the deep Lockman Hole survey. The goal of the classification has been the separation of the sources into Galactic and extragalactic objects. For this purpose, we have used the results of our previous cross-match of X-ray sources with optical catalogs. For the classificat…

2022 Astronomy Letters
Gaia 1