Zobrazeno 1 - 10
of 40
pro vyhledávání: '"Aleksandr A. Boyarchuk"'
Publikováno v:
Solar System Research. 47:499-507
The “Spektr-UF” project is intended for the design and development of a large space observatory operating in the ultraviolet (UV) band of the spectrum inaccessible for survey from the surface of the Earth. The main observatory instrument is a spa
Publikováno v:
Physics-Uspekhi. 55:115-136
The current understanding of mass exchange processes between close binary system (CBS) components is reviewed, with particular attention on the mass flow structure and accretion disk physics. Using 3D MHD calculation results, the variation of key acc
Publikováno v:
Astronomy Reports. 53:660-674
We present the results of a comparative analysis of the atmospheric chemical abundances of red giants in several open clusters: the Hyades, Collinder 350, NGC 6475, and Ruprecht 147. We determined the atmospheric parameters of all the stars and the e
Publikováno v:
Chinese Journal of Astronomy and Astrophysics. 6:159-163
The three-dimensional gas dynamic simulations in SU UMa-type binaries show the formation of the precessional spiral density wave in inner parts of the accretion disk that are not subjected to gas dynamic perturbations. The features of the precessiona
Autor:
A. M. Cherepashchuk, Dmitry Bisikalo, O. A. Kuznetsov, T. S. Khruzina, Aleksandr A. Boyarchuk
Publikováno v:
Astronomy Reports. 49:79-88
We have analyzed the orbital light curve of the X-ray nova XTE J1118+480 in a “disk + hot line” model based on three-dimensional gas-dynamical computations of gas flows in interacting binary systems. As a result, we have been able to derive relia
Autor:
D G Yakovlev, A A Kaplyansky, R L Aptekar, K A Konoplev, A G Zabrodsky, D. A. Varshalovich, Lev Zelenyi, R. A. Sunyaev, Aleksandr A. Boyarchuk, Robert A. Suris, G S Bisnovatyi-Kogan, Andrei M. Bykov
Publikováno v:
Physics-Uspekhi. 56:1150-1152
Publikováno v:
Astronomy Reports. 47:809-820
We analyze heating and cooling processes in accretion disks in binaries. For realistic parameters of the accretion disks in close binaries ( $$\dot M \simeq 10^{ - 12} - 10^7 M_ \odot /yr$$ and α⋍10−1–10−2), the gas temperature in the outer
Autor:
Aleksandr A. Boyarchuk, O. A. Kuznetsov, A. M. Cherepashchuk, Dmitry Bisikalo, T. S. Khruzina
Publikováno v:
Astronomy Reports. 47:621-636
We have analyzed optical and infrared light curves of GU Mus obtained during the system's quiescent state and carried out computations for “hot-line” and “hot-spot” models. The hot-line model describes the optical variability of GU Mus better
Autor:
Dmitry Bisikalo, A. M. Cherepashchuk, Aleksandr A. Boyarchuk, O. A. Kuznetsov, T. S. Khruzina
Publikováno v:
Astronomy Reports. 47:214-231
To determine the parameters of the accretion disk and shock-wave region responsible for the formation of the orbital peak in the light curve of the binary system OY Car (an SU UMa-type variable), we have analyzed its U BV R and JK light curves using
Autor:
Anatolii M. Cherepashchuk, D. A. Varshalovich, Aleksandr A. Boyarchuk, R. A. Syunyaev, Vladimir V. Kocharovsky, Vladimir I Talanov, I.E. Trümper, Evgenii A Mareev, Andrei V. Gaponov-Grekhov, Aleksandr F. Andreev, Aleksandr Grigorievich Litvak, Lev Zelenyi
Publikováno v:
Physics-Uspekhi. 54:109-111