Zobrazeno 1 - 10
of 173
pro vyhledávání: '"A. A. Kilpio"'
Autor:
A. A. Kilpio
Publikováno v:
Odessa Astronomical Publications, Vol 14, Iss 0, Pp 38-40 (2017)
The results of 3D numerical simulations of mass transfer in semidetached binaries after the mass transfer termination are presented. On the first stage the 3D gasdynamical simulation of mass transfer for the case of constant rate of mass transfer has
Externí odkaz:
https://doaj.org/article/713131c73cc94fe1b8b71e641643852a
Akademický článek
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Results of the study of the symbiotic binary Z And during its recent active phase 2000 -- 2010 when it experienced a series of six optical outbursts are presented. High-resolution spectra obtained during the first and fourth outburst, which was the s
Externí odkaz:
http://arxiv.org/abs/1012.2803
Publikováno v:
Astron.Rep. 80 (2006) 722-732
Two-dimensional gas-dynamical modeling of the mass-flow structure is used to study the outburst development in the classical symbiotic star Z And. The stage-by-stage rise of the light during the outburst can be explained in the framework of the colli
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610415
Autor:
Mitsumoto, M., Jahanara, B., Matsuda, T., Oka, K., Bisikalo, D. V., Kilpio, E. Yu., Boffin, H. M. J., Boyarchuk, A. A., Kuznetsov, O. A.
Publikováno v:
Astron.Rep.49:884-891,2005
The results of 3D modelling of the flow structure in the classical symbiotic system Z~Andromedae are presented. Outbursts in systems of this type occur when the accretion rate exceeds the upper limit of the steady burning range. Therefore, in order t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0510175
Results of calculations of the flow structure in binary systems with mass exchange driven by stellar wind are presented. 2D simulations have been carried out using the Roe-Oscher scheme. The fine grid we used allowed us to detect the details of the f
Externí odkaz:
http://arxiv.org/abs/astro-ph/0212227
The results of three-dimensional numerical simulations of mass transfer in binaries with spiral shocks are presented. It is shown that the mass transfer rate variation disturbs the equilibrium state of accretion disk and results in formation of the b
Externí odkaz:
http://arxiv.org/abs/astro-ph/0105403
Publikováno v:
Astron. Zh. 2001, v.78, pp.707-716 (Astron. Reports, v.45, pp.611-619)
The results of three-dimensional numerical simulations of mass transfer in semidetached binaries after mass transfer termination is presented and the structure of residual accretion disk was investigated. It was shown that after the mass transfer ter
Externí odkaz:
http://arxiv.org/abs/astro-ph/0102241
Autor:
Malkov Oleg, Karpov Sergey, Kilpio Elena, Sichevsky Sergey, Chulkov Dmitry, Dluzhnevskaya Olga, Kovaleva Dana, Kniazev Alexei, Mickaelian Areg, Mironov Alexey, Murthy Jayant, Sytov Alexey, Zhao Gang, Zhukov Aleksandr
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://doaj.org/article/d49103bf5de44a26a17e084b284dba09
Autor:
E. Yu. Kilpio, I. A. Shcherbakov
Publikováno v:
Doklady Physics. 67:377-404
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::093de8f88b57553088d83e71992ad346
https://doi.org/10.1134/s1028335822100068
https://doi.org/10.1134/s1028335822100068