Search Publications

Physical and Dynamical Parameters of the Triple Stellar System: HIP 109951
DOI: 10.1134/S1990341319040126 Bibcode: 2019AstBu..74..464M

Docobo, J. A.; Hussein, A. M.; Mardini, M. K. +5 more

The precise determination of the physical and dynamical parameters of the HIP 109951 triple star system (WDS J22161-0705AB) which is formed by the A, Ba, and Bb components are presented. The binary nature of component B was recently confirmed by studying the radial velocities. The analysis of the system follows Al-Wardat's complex method for analy…

2019 Astrophysical Bulletin
Hipparcos 21
Unity and Diversity of Yellow Hypergiants Family
DOI: 10.1134/S1990341319040138 Bibcode: 2019AstBu..74..475K

Klochkova, V. G.

We present the results of long-term spectral monitoring of yellow hypergiants (YHGs) of northern hemisphere with a R ≥ 60 000 resolution. The spectra of these F–G stars of extreme luminosity, compactly located at the top of the Hertzsprung–Russell diagram revealed a variety of spectral features: various types of Hα profile, the presence (or absenc…

2019 Astrophysical Bulletin
Gaia 13
Kinematics of Open Star Clusters Based on the Data of the New Version of the "Homogeneous Catalog of Open Cluster Parameters"
DOI: 10.1134/S1990341319030039 Bibcode: 2019AstBu..74..270L

Loktin, A. V.; Popova, M. E.

We investigate some aspects of Galactic disc kinematics based on the data on open clusters from the current version of "The Homogeneous Catalog of the Main Parameters of Open Star Clusters" and from Gaia DR2. Based on the radial velocity and proper motion data for the clusters we determine the angular velocity of the Sun in the Galaxy as Ω0

2019 Astrophysical Bulletin
Gaia 12
Spectroscopy of Supergiants with Infrared Excess: Results of 1998–2018
DOI: 10.1134/S1990341319020032 Bibcode: 2019AstBu..74..140K

Klochkova, V. G.

We shortly summarize here the results of the second stage (1998–2018) of the detailed spectroscopy program of peculiar supergiants identified with galactic infrared sources, performed at the 6-m BTA telescope. The main aspect of the program is a search for the evolutionary variations in the chemical composition of stars, past the AGB stage and the…

2019 Astrophysical Bulletin
Gaia 3
Optical Spectrum of Distant OH/IR Star V1648 Aql (IRAS 19386+0155)
DOI: 10.1134/S1990341319030040 Bibcode: 2019AstBu..74..277K

Klochkova, V. G.; Tavolzhanskaya, N. S.

We present an optical spectrum of the star V1648 Aql (IRAS19386+0155) obtained at the 6-m SAO RAS telescope with a spectral resolution of R ≥ 60 000. Heliocentric radial velocity was measured from numerous metal absorptions is Vr = 10.18 ± 0.05 km s-1 (VLSR = 18.1 km s-1). We determined the atmospheric, …

2019 Astrophysical Bulletin
Gaia 3
CCD Observations and Period Change of the Type ab RR Lyrae Star DV Mon
DOI: 10.1134/S199034131902007X Bibcode: 2019AstBu..74..183B

Dambis, A. K.; Berdnikov, L. N.; Kniazev, A. Yu. +3 more

We took a total of 635 B-, V-, and Ic-band CCD frames for the RRab Lyr type variable DVMon, which has a close bright visual companion with a separation of about 1.9'. Observations were made with the 76-cm telescope of the South African Astronomical Observatory (SAAO, South Africa) using SBIG CCD ST-10XME. For the first time, we obtained…

2019 Astrophysical Bulletin
Gaia INTEGRAL 2
Long-Term Activity of a Little Known Dwarf Nova DT Octantis
DOI: 10.1134/S199034131904014X Bibcode: 2019AstBu..74..490S

Šimon, V.; Edelmann, H.

We analyze the long-term activity of a little known dwarf nova (DN) DT Oct. We use photographic observations from the Bamberg Observatory (Southern Patrol Photographic Sky Survey), CCD data from ASAS-3 survey, and AAVSO data (both CCD and visual). We determined the recurrence times of the superoutbursts, TCso, and of the normal outburst…

2019 Astrophysical Bulletin
Gaia 1
Search for Possibly Evolutionary Linked Globular and Open Clusters
DOI: 10.1134/S1990341319010036 Bibcode: 2019AstBu..74...29B

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

Based on a large sample of 133 Galactic globular clusters we obtained a new estimate of the frequency of globular-cluster impacts onto the Galactic plane, which we found to be equal to three events per 1 Myr. Our computations involving new kinematical data do not support the well-known hypothesis about the possible origin of the open cluster Steph…

2019 Astrophysical Bulletin
Gaia 1
SEROB1A Association in DR2 GAIA Epoch
DOI: 10.1134/S1990341319020068 Bibcode: 2019AstBu..74..179C

Chentsov, E. L.

In the light of new astrometric and available spectroscopic data, the structure and kinematics of the SerOB1A association are discussed and the issue of correcting its boundaries is put.

2019 Astrophysical Bulletin
Gaia 1