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pro vyhledávání: '"A. A. Kilpio"'
Akademický článek
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Autor:
E. G. Stanley
Publikováno v:
Notes and Queries. 59:584-588
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e576e4c1f3192cfdb70b05b2fadf02fa
https://doi.org/10.1093/notesj/gjs189
https://doi.org/10.1093/notesj/gjs189
Autor:
Mark Faulkner
Publikováno v:
Notes and Queries. 58:606-608
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9b3b30c64f98e4171ae5b9a9cb3a0d48
https://doi.org/10.1093/notesj/gjr194
https://doi.org/10.1093/notesj/gjr194
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