Study of the non-stationarity of the atmosphere of κ Cas. Ii. Variability of the Hγ, Hβ, and Hα wind-line profilesAstrophysical Bulletin - Tập 72 - Trang 452-457 - 2017
A. Kh. Rzaev
We study the variability of the Hγ, Hβ, and Hα line profiles in the spectrum of
the supergiant κ Cas. The variability pattern proved to be the same for all the
lines considered: their profiles are superimposed by blueshifted, central, and
redshifted emission. For Hγ the positions of the emissions coincide with the
positions of the corresponding emissions for He I λλ 5876, 6678 Å lines, and are
equ... hiện toàn bộ
Search for possible connections between isolated radio pulsars and supernova remnantsAstrophysical Bulletin - Tập 67 - Trang 160-176 - 2012
E. G. Chmyreva, G. M. Beskin, A. V. Biryukov
We have developed a method of searching for the connections between the isolated
radio pulsars and supernova remnants, based on the analysis of their kinematic
characteristics. We investigate fairly young (τ ch ≲ 106 yr) radio pulsars with
known proper motions and estimated distances (dispersion measures), and
supernova remnants located no more than 1–2 kpc away from them. Using a standard
empiric... hiện toàn bộ
Database for Studying Edge-on GalaxiesAstrophysical Bulletin - Tập 76 - Trang 218-227 - 2021
D. I. Makarov, A. V. Antipova
Abstract—We present a database created within the project on studying edge-on
galaxies. These galaxies provide a unique opportunity to study the
three-dimensional distribution of the matter in galaxy disks, which is extremely
important for analyzing the influence of internal and external factors on the
evolution of galaxies. For the moment, extensive observed material has been
accumulated on the k... hiện toàn bộ
Speckle interferometry of nearby multiple stars. V. 2002–2006 positional measurementsAstrophysical Bulletin - Tập 68 - Trang 53-56 - 2013
I. I. Balega, Yu. Yu. Balega, L. T. Gasanova, V. V. Dyachenko, A. F. Maksimov, E. V. Malogolovets, D. A. Rastegaev, Z. U. Shkhagosheva
We present the measurements of positional parameters of 194 nearby binary stars
performed at the 6-m BTA telescope of the SAO RAS from 2002 through 2006
applying the speckle interferometric technique. The observations were conducted
at central filter wavelengths ranging from 545 to 800 nm using a speckle
interferometer equipped with a fast CCD and a three-stage image intensifier. A
significant par... hiện toàn bộ
Studies of Features of Evolution of Highly Magnetized Stars—White Dwarfs. I. ObservationsAstrophysical Bulletin - Tập 77 - Trang 301-307 - 2022
V. N. Aitov, G. G. Valyavin, A. F. Valeev, G. Sh. Mitiani, A. S. Moskvitin, E. B. Emelyanov, T. A. Fatkhullin, K. A. Antonyuk, G. A. Galazutdinov, A. R. Zakinyan, S. A. Kunikin
We present the results of observations within the program for the search for new
highly magnetized white dwarfs among evolutionary old stars of this class. The
program was carried out for two years at the 1-m telescope of the SAO RAS. As a
result, new white dwarf candidates of different ages with super-strong (several
megagauss, tens, hundreds of megagauss) magnetic fields were discovered. These
o... hiện toàn bộ
Analysis of the properties of clusters of galaxies in the region of the Ursa Major superclusterAstrophysical Bulletin - Tập 64 - Trang 1-23 - 2009
F. G. Kopylova, A. I. Kopylov
We analyze the properties of the clusters of galaxies in the region of the Ursa
Major (UMa) supercluster using observational data from SDSS and 2MASS catalogs.
The region studied includes a supercluster (with a galaxy and cluster
overdensity of 3 and 15, respectively) and field clusters inside the 150-Mpc
diameter surrounding region. The total dynamical mass of 10 clusters of galaxies
in UMa is eq... hiện toàn bộ
Parameters of SU UMa and WZ Sge-Type Dwarf Novae in Quiescent State. I. FL Psc, TY Psc and V455 AndAstrophysical Bulletin - Tập 78 - Trang 25-35 - 2023
A. A. Dudnik, V. V. Shimansky, N. V. Borisov, A. A. Mitrofanova, M. M. Gabdeev
We present the results of model analysis of the optical spectra of SU UMa and WZ
Sge-type dwarf novae TY Psc, FL Psc, and V455 And. Spectroscopic observations
were carried out at the SAO RAS 6-m BTA telescope in 2013. The selection
criterion for the systems under study is their existence in a quiescent state
with an optically thin accretion disk and dominance of white dwarf radiation.
The fulfillm... hiện toàn bộ