排序方式： 共有11条查询结果，搜索用时 15 毫秒
1.
Cherepashchuk A. M. Dodin A. V. Postnov K. A. Belinski A. A. Burlak M. A. Ikonnikova N. P. Irsmambetova T. R. Trushkin S. A. 《Astronomy Reports》2022,66(6):451-465
Astronomy Reports - The observed characteristics of the spectral and photometric variability of SS 433 are discussed based on the data for 2018–2021 and compared with earlier results. The... 相似文献
2.
Victor G. Kornilov Vladimir M. Lipunov Evgeny S. Gorbovskoy Aleksander A. Belinski Dmitry A. Kuvshinov Natalia V. Tyurina Nikolai I. Shatsky Anatoly V. Sankovich Aleksander V. Krylov Pavel V. Balanutsa Vadim V. Chazov Artem S. Kuznetsov Dmitry S. Zimnuhov Victor A. Senik Andrey G. Tlatov Aleksander V. Parkhomenko Denis V. Dormidontov Vadim V. Krushinsky Ivan S. Zalozhnyh Aleksander A. Popov Sergey A. Yazev Nikolai M. Budnev Kirill I. Ivanov Evgeny N. Konstantinov Oleg A. Gress Oleg V. Chvalaev Vladimir V. Yurkov Yury P. Sergienko Irina P. Kudelina 《Experimental Astronomy》2012,33(1):173-196
Presented paper describes the basic principles and features of the implementation of a robotic network of optical telescopes MASTER, designed to study the prompt (simultaneous with gamma radiation) optical emission of gamma-ray bursts and to perform the sky survey to detect unknown objects and transient phenomena. With joint efforts of Sternberg astronomical institute, High altitude astronomical station of the Pulkovo observatory, Ural state university, Irkutsk state university, Blagoveshchensk pedagogical university, the robotic telescopes MASTER?II near Kislovodsk, Yekaterinburg, Irkutsk and Blagoveshchensk were installed and tested. The network spread over the longitudes is greater than 6?h. A further expansion of the network is considered. 相似文献
3.
Dodin A. V. Potanin S. A. Shatsky N. I. Belinski A. A. Atapin K. E. Burlak M. A. Egorov O. V. Tatarnikov A. M. Postnov K. A. Belvedersky M. I. Burenin R. A. Gilfanov M. R. Medvedev P. S. Meshcheryakov A. V. Sazonov S. Yu. Khorunzhev G. A. Sunyaev R. A. 《Astronomy Letters》2020,46(7):429-438
Astronomy Letters - Based on observations with the new transient double-beam spectrograph (TDS) at the 2.5-m telescope of the Caucasus Mountain Observatory of SAI MSU, we have determined the types... 相似文献
4.
Sergei V.Antipin Ignacio Becker AlexANDer A.Belinski Darya M.Kolesnikova Karim Pichara Nikolay N.Samus Kirill V.Sokolovsky Alla V.Zharova Alexandra M.Zubareva 《天文和天体物理学研究(英文版)》2018,(8)
Using 172 plates taken with the 40-cm astrograph of the Sternberg Astronomical Institute(Lomonosov Moscow University) in 1976–1994 and digitized with a resolution of 2400 dpi, we discovered and studied 275 new variable stars. We present the list of our new variables with all necessary information concerning their brightness variations. As in our earlier studies, the new discoveries show a rather large number of high-amplitude Delta Scuti variables, predicting that many stars of this type remain not detected in the whole sky. We also performed automated classification of the newly discovered variable stars based on the Random Forest algorithm. The results of the automated classification were compared to traditional classification and showed that automated classification was possible even with noisy photographic data. However, further improvement of automated techniques is needed, which is especially important when considering the very large numbers of new discoveries expected from all-sky surveys. 相似文献
5.
Dodin A. V. Shatsky N. I. Belinski A. A. Atapin K. E. Burlak M. A. Zheltoukhov S. G. Tatarnikov A. M. Postnov K. A. Cherepashchuk A. M. Belvedersky M. I. Borisov V. D. Burenin R. A. Gilfanov M. R. Krivonos R. A. Medvedev P. S. Meshcheryakov A. V. Sazonov S. Yu. Sunyaev R. A. Khorunzhev G. A. 《Astronomy Letters》2021,47(10):661-673
Astronomy Letters - Based on observations with the transient double-beam spectrograph (TDS) at the 2.5-m telescope of the Caucasus Mountain Observatory of SAI MSU, we have determined the redshifts... 相似文献
6.
Antipin S. V. Zubareva A. M. Belinski A. A. Burlak M. A. Ikonnikova N. P. Sokolovsky K. V. 《Astronomy Letters》2020,46(10):677-690
Astronomy Letters - Results of the first multicolor photometric observations of the unusual dwarf nova V2466 Cygni during its 2003 and 2019 superoutbursts are presented. The total amplitude of the... 相似文献
7.
M. V. Barkov V. A. Belinski G. S. Bisnovatyi-Kogan 《Monthly notices of the Royal Astronomical Society》2002,334(2):338-344
It is shown that during the motion of two initially gravitationally bound spherical shells, consisting of point particles moving along ballistic trajectories, one of the shells may be expelled to infinity at subrelativistic speed v exp ≤0.25 c . The problem is solved in Newtonian gravity. Motion of two intersecting shells in the case when they do not runaway shows a chaotic behaviour. We hope that this toy and oversimplified model can nevertheless give a qualitative idea on the nature of the mechanism of matter outbursts from dense stellar clusters . 相似文献
8.
E. S. Gorbovskoy V. M. Lipunov V. G. Kornilov A. A. Belinski D. A. Kuvshinov N. V. Tyurina A. V. Sankovich A. V. Krylov N. I. Shatskiy P. V. Balanutsa V. V. Chazov A. S. Kuznetsov A. S. Zimnukhov V. P. Shumkov S. E. Shurpakov V. A. Senik D. V. Gareeva M. V. Pruzhinskaya A. G. Tlatov A. V. Parkhomenko D. V. Dormidontov V. V. Krushinsky A. F. Punanova I. S. Zalozhnyh A. A. Popov A. Yu. Burdanov S. A. Yazev N. M. Budnev K. I. Ivanov E. N. Konstantinov O. A. Gress O. V. Chuvalaev V. V. Yurkov Yu. P. Sergienko I. V. Kudelina E. V. Sinyakov I. D. Karachentsev A. V. Moiseev T. A. Fatkhullin 《Astronomy Reports》2013,57(4):233-286
The main stages in the creation of the Russian segment of the MASTER network of robotic telescopes is described. This network is designed for studies of the prompt optical emission of gammaray bursts (GRBs; optical emission synchronous with the gamma-ray radiation) and surveys of the sky aimed at discovering uncataloged objects and photometric studies for various programs. The first results obtained by the network, during its construction and immediately after its completion in December 2010, are presented. Eighty-nine alert pointings at GRBs (in most cases, being the first ground telescopes to point at the GRBs) were made from September 2006 through July 2011. The MASTER network holds first place in the world in terms of the total number of first pointings, and currently more than half of first pointings at GRBs by ground telescopes are made by the MASTER network. Photometric light curves of GRB 091020, GRB 091127, GRB 100901A, GRB 100906A, GRB 10925A, GRB 110106A, GRB 110422A, and GRB 110530A are presented. It is especially important that prompt emission was observed for GRB 100901A and GRB 100906A, and thar GRB 091127, GRB 110422A, and GRB 110106A were observed from the first seconds in two polarizations. Very-wide-field cameras carried out synchronous observations of the prompt emission of GRB 081102, GRB 081130B, GRB 090305B, GRB 090320B, GRB 090328, and GRB 090424. Discoveries of Type Ia supernovae are ongoing (among them the brightest supernova in 2009): 2008gy, 2009nr, 2010V, and others. In all, photometry of 387 supernovae has been carried out, 43 of which were either discovered or first observed with MASTER telescopes; more than half of these are Type Ia supernovae. Photometric studies of the open clusters NGC 7129 and NGC 7142 have been conducted, leading to the discovery of 38 variable stars. Sixty-nine optical transients have been discovered. 相似文献
9.
V. M. Lipunov V. G. Kornilov A. V. Krylov G. V. Borisov D. A. Kuvshinov A. A. Belinski E. S. Gorbovskoy G. A. Antipov N. V. Tyurina V. M. Vitrischak S. A. Potanin M. V. Kuznetsov 《Astrophysics》2005,48(3):389-399
The operating principles of the telescope-robot system MASTER (Mobile Astronomical System of Telescopes-Robots, http://observ.pereplet.ru), designed to search for fast transient phenomena in the optical range, are described. The robot-telescope includes the following: a Richter-Slefogt telescope with D=355 mm, F/D=2.4, a Richter-Slefogt telescope with D=200 mm, F/D=2.4, a Flugge telescope with D=280 mm, F/D=2.5, a TV camera with a field of 20x40 degrees, and three CCD cameras. A German mount with a slew rate of 8 deg/s is used. MASTER obtains images down to 19m in a field of 6 square degrees in a 1.5 minute exposure. We present some observations of the optical afterglow of cosmic gamma-ray bursts. MASTER was the first system in Europe to record optical emission from GRB030329.__________Translated from Astrofizika, Vol. 48, No. 3, pp. 463–475 (August 2005). 相似文献
10.
V. M. Lipunov V. G. Kornilov E. S. Gorbovskoy A. V. Krylov N. V. Tyurina D. A. Kuvshinov A. A. Belinski P. A. Gritsyk A. V. Sankovich V. V. Vladimirov 《Astronomy Letters》2008,34(3):145-151
The MASTER robotic telescope has obtained the first optical images of GRB 060926. We have discovered an optical flare from GRB 060926, a recurrent brightening that closely follows its behavior in the X-ray range. We have determined the spectral slope for GRB 060926 from the X-ray to optical range in the first minutes. Based on the spinar model, we show that the parameters of the optical and X-ray flares suggest that the gamma-ray burst resulted from the core collapse of a 7M ⊙ star with an initial effective Kerr parameter of 7.6 and an initial magnetic-to-gravitational energy ratio of 10?4. 相似文献