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Simultaneous X-ray/UV Observations of Ultraluminous X-ray Source Holmberg II X-1 with Indian Space Mission Astrosat
DOI: 10.1134/S1990341322030129 Bibcode: 2022AstBu..77..231V

Vinokurov, A.; Solovyeva, Y.; Atapin, K. +11 more

We present the results of eight epochs of simultaneous UV and X-ray observations of the highly variable ultraluminous X-ray source (ULX) Holmberg II X-1 with AstroSat—Indian multiwavelength space satellite. During the entire observation period from late 2016 to early 2020, Holmberg II X-1 showed a moderate X-ray luminosity about of

2022 Astrophysical Bulletin
XMM-Newton 3
Discovery of New δ Scuti Stars
DOI: 10.1134/S1990341322030051 Bibcode: 2022AstBu..77..316K

Kιrmιzιtaş, Ö.; Çavuş, S.; Aliçavuş, F. Kahraman

—Pulsating stars are remarkable objects for stellar astrophysics. Their pulsation frequencies allow us to probe the internal structure of stars. One of the most known groups of pulsating stars is $$\delta $$ Scuti variables which could be used to understand the energy tr…

2022 Astrophysical Bulletin
Gaia 3
Detailed Spectroscopy of Post-AGB Supergiant GSC 04050–02366 in IRAS Z02229+6208 IR Source System
DOI: 10.1134/S1990341322030063 Bibcode: 2022AstBu..77..292K

Klochkova, V. G.; Panchuk, V. E.

—In the optical spectra of the cold post-AGB supergiant GSC $$04050$$$$02366$$, obtained with the 6‑m BTA telescope with a resolution of $$R \…

2022 Astrophysical Bulletin
Gaia 2
Tidal Constraints for Wide Binaries in Pleiades
DOI: 10.1134/S199034132202002X Bibcode: 2022AstBu..77..182D

Danilov, V. M.

—A technique is proposed for estimating the parameters of spatial orientation of the $${{{\mathbf{r}}}_{{1,2}}}$$ vectors of distances between the components in wide binary stars (BS) in open star clusters (OCs). An analysis of the orientation features of these vectors f…

2022 Astrophysical Bulletin
Gaia 1
Activity of the Young Star TOI 837 with an Exoplanet
DOI: 10.1134/S1990341322040113 Bibcode: 2022AstBu..77..431S

Savanov, I. S.

—Based on high-precision data from the archive of the TESS space mission, a study was made of the photometric brightness variability of TOI 837—a young star with an exoplanet, a member of the southern sky cluster IC 2602. Based on all available observational results, we have estimated the star's rotation period and brightness variability amplitude…

2022 Astrophysical Bulletin
Gaia 1
Mass of the Asteroid (7348) 1993FJ22 as Determined by the Dynamic Method
DOI: 10.1134/S1990341322010072 Bibcode: 2022AstBu..77..112K

Kuznetsov, V. B.; Chernetenko, Yu. A.

—The mass of the asteroid ($$7348$$) is determined by the dynamic method based on the analysis of gravitational perturbations in the motion of the asteroid (7562) Kagiroino–Oka caused by asteroid (7348). The choice of these asteroids is due to the fact that on March

2022 Astrophysical Bulletin
Gaia 0
Photometric Study of the Open Cluster NGC 225
DOI: 10.1134/S1990341322010126 Bibcode: 2022AstBu..77...78Y

Carraro, G.; Ikonnikova, N. P.; Yalyalieva, L. N. +2 more

—NGC 225 is a young moderately populated cluster with discrepant age, distance, and color excess estimates reported by different authors. We combine our photometry with the data from large surveys (2MASS, WISE, Pan-STARRS) to derive the parameters of NGC 225 and study the extinction law in the near infrared in the direction of the cluster. We use …

2022 Astrophysical Bulletin
Gaia 0