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Article
WSO–UV Project: New Touches
Abstract—A general description is given of the international (with Russia as the key contributor) project World Space Observatory–Ultraviolet (WSO–UV; in Russian named SPEKTR–UF). The project is aimed at creating...
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Article
Evolution of the accretion structure of the compact object in the symbiotic binary BF Cygni during outburst in 2009–2014
The eclipsing symbiotic binary BF Cyg has had five orbital minima during its last optical outburst after 2006. The second minimum is much shallower than the first one and after that the minimum get deeper agai...
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Article
Changes in the Martian atmosphere induced by auroral electron precipitation
Typical auroral events in the Martian atmosphere, such as discrete and diffuse auroral emissions detected by UV spectrometers onboard ESA Mars Express and NASA MAVEN, are investigated. Auroral electron kinetic en...
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Article
Monte Carlo study of interaction between solar wind plasma and Venusian upper atmosphere
Isolated events of proton and alpha particle precipitation in the Venusian atmosphere were recorded with the use of the ASPERA-4 analyzer on board the ESA Venus Express spacecraft. Using a Monte Carlo simulati...
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Article
Ionization fraction in the thermosphere of the exoplanet HD 209458b
Dissociation and ionization of hydrogen molecules and ionization of hydrogen atoms due to extreme UV radiation from the parent star are accompanied by the formation of a concurrent photoelectron flux with exce...
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Article
Gaseous flows in the inner part of the circumbinary disk of the T Tauri star
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 th...
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Article
Influence of the hot oxygen corona on the satellite drag in the Earth’s upper atmosphere
Calculation results on the possible influence of the hot oxygen fraction on the satellite drag in the Earth’s upper atmosphere on the basis of the previously developed theoretical model of the hot oxygen geoco...
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Article
On Possible Nature of Pre-eclipse Dips in Light Curves of Semi-detached Systems with Steady-state Disks
In order to explain pre-eclipse dips at phases ~0.7 in light curves of cataclysmic variables, the hypothesis of the thickening at the outer edge of the accretion disk is usually used. Shock-free nature of the ...
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Chapter and Conference Paper
The Morphology of Gaseous Flows in Z and in the Active State
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Chapter and Conference Paper
Morphology of the Interaction between the Stream and Cool Accretion Disc in Semidetached Binaries
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Chapter and Conference Paper
Disc Formation in Binary be Stars
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Article
Numerical Modeling of Mass Transfer in Close Binaries
The review of gasdynamic models used for the description of the mass exchange in close binaries is presented. Main features of the flow structure are summarized. Special attention is paid to physics of accreti...
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Article
Summary of quantitative interpretation of IMAGE far ultraviolet auroral data
Direct imaging of the magnetosphere by instruments on the IMAGE spacecraft is supplemented by simultaneous observations of the global aurora in three far ultraviolet (FUV) wavelength bands. The purpose of the ...
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Chapter
Summary of Quantitative Interpretation of IMAGE Far Ultraviolet Auroral Data
Direct imaging of the magnetosphere by instruments on the IMAGE spacecraft is supplemented by simultaneous observations of the global aurora in three far ultraviolet (FUV) wavelength bands. The purpose of the ...
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Article
Gasdynamical Treatment of Mass Transfer in Symbiotic Stars
The results of two-dimensional, non-adiabatic gas dynamical simulations of gas flows in symbiotic stars are presented. It is shown that for a binary system with components that do not fill their Roche lobes, t...