Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Alexey Sytov"'
Autor:
Oleg Malkov, Sergey Karpov, Dana Kovaleva, Sergey Sichevsky, Dmitry Chulkov, Olga Dluzhnevskaya, Alexey Kniazev, Areg Mickaelian, Alexey Mironov, Jayant Murthy, Alexey Sytov, Gang Zhao, Aleksandr Zhukov
Publikováno v:
Galaxies, Vol 7, Iss 1, p 7 (2018)
Results of comparison of Gaia DR2 parallaxes with data derived from a combined analysis of 2MASS (Two Micron All-Sky Survey), SDSS (Sloan Digital Sky Survey), GALEX (Galaxy Evolution Explorer), and UKIDSS (UKIRT Infrared Deep Sky Survey) surveys in f
Externí odkaz:
https://doaj.org/article/b0f485b3c6e946228cff4f4e04e70ea6
Autor:
Alexey Sytov, Sergey Karpov, Jayant Murthy, A. Y. Kniazev, Oleg Malkov, Sergey Sichevsky, D. A. Chulkov, O. B. Dluzhnevskaya, Elena Kilpio, Dana Kovaleva, A. V. Mironov, A. O. Zhukov, Gang Zhao, Areg M. Mickaelian
Publikováno v:
Open Astronomy, Vol 27, Iss 1, Pp 62-69 (2018)
Information on interstellar extinction and dust properties may be obtained from modern large photometric surveys data. Virtual Observatory facilities allow users to make a fast and correct cross-identification of objects from various surveys. It yiel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b262eb2da46f65d907cfd432ec0751fc
https://doi.org/10.1515/astro-2018-0002
https://doi.org/10.1515/astro-2018-0002
Autor:
Lev R. Yungelson, Oleg Malkov, D. A. Chulkov, Alexander V. Tutukov, Nikolay A. Skvortsov, Dana Kovaleva, Y. M. Gebrehiwot, Solomon Belay Tessema, Alexey Sytov
Publikováno v:
Communications in Computer and Information Science ISBN: 9783030235833
DAMDID/RCDL (Selected Papers)
DAMDID/RCDL (Selected Papers)
Creation of the Galaxy model describing formation and evolution of binary stars requires generating and testing hypotheses related to the process of formation of binary stars and distributions of their characteristics. A set of hypotheses can be gene
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d1c95c10ede65811920edfac20d623e7
https://doi.org/10.1007/978-3-030-23584-0_6
https://doi.org/10.1007/978-3-030-23584-0_6
Autor:
Areg M. Mickaelian, Alexey Sytov, Jayant Murthy, Gang Zhao, A. O. Zhukov, Oleg Malkov, Dana Kovaleva, O. B. Dluzhnevskaya, Sergey Sichevsky, Alexey Kniazev, A. V. Mironov, Sergey Karpov, D. A. Chulkov
Publikováno v:
Galaxies, Vol 7, Iss 1, p 7 (2018)
Galaxies
Volume 7
Issue 1
Galaxies
Volume 7
Issue 1
Results of comparison of Gaia DR2 parallaxes with data derived from a combined analysis of 2MASS (Two Micron All-Sky Survey), SDSS (Sloan Digital Sky Survey), GALEX (Galaxy Evolution Explorer), and UKIDSS (UKIRT Infrared Deep Sky Survey) surveys in f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7452e7475a6bdc35b5756c472cb4ab71
Publikováno v:
Astrophysics and Space Science. 335:125-129
We present results of 3D numerical simulations of the matter flow in the disk of a binary T Tauri star. It is shown that two bow-shocks caused by the supersonic motion of the binary components in the gas of the disk are formed in the system having pa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0d1238835070ab720138f7f0b7aaf4e6
https://doi.org/10.1007/s10509-011-0601-5
https://doi.org/10.1007/s10509-011-0601-5
Publikováno v:
The Astrophysical Journal. 818:L17
Young solar-type stars grow through the accretion of material from the circumstellar disk during pre-main sequence (PMS) evolution. The ultraviolet radiation generated in this process plays a key role in the chemistry and evolution of young planetary
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8759712b8ba1f1d78e4a6fe49f0cdbe
https://doi.org/10.3847/2041-8205/818/1/l17
https://doi.org/10.3847/2041-8205/818/1/l17
Publikováno v:
Proceedings of the International Astronomical Union. 7:547-548
We have carried out 2D and 3D numerical simulations (Kaigorodov et al. 2010, Fateeva et al. 2011, Sytov et al. 2011) of accretion processes in binary T Tauri stars (TTSs) DQ Tau, UZ Tau E, V4046 Sgr, GW Ori, RoXs 42C using a finite-difference Roe-Osh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::711742d2a53b690ca66fdb3d132f66a7
https://doi.org/10.1017/s1743921311028353
https://doi.org/10.1017/s1743921311028353