Search Results - "Bisikalo, D V"
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Monte Carlo model of electron transport for the calculation of Mars dayglow emissions
Published in Journal of Geophysical Research - Planets (01-02-2008)“…A model of the photoelectron collision‐induced component of the Mars dayglow using recent cross sections and solar flux is described. The calculation of the…”
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Full 3D MHD calculations of accretion flow structure in magnetic cataclysmic variables with strong, complex magnetic fields
Published in Astronomy reports (01-04-2012)“…We have performed three-dimensional magnetohydrodynamical calculations of stream accretion in cataclysmic variable stars for which the white dwarf primary…”
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The role of atmospheric outflows in the migration of hot Jupiters
Published in Monthly notices of the Royal Astronomical Society (01-09-2021)“…ABSTRACT Many of observed hot Jupiters are subject to atmospheric outflows. Numerical simulations have shown that the matter escaping from the atmosphere can…”
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Shock propagation in accretion discs around merging black holes: self-similar solution
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…ABSTRACT To date, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the Virgo gravitational wave detectors have registered several events due…”
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Atmospheric Mass Loss from Hot Jupiters Irradiated by Stellar Superflares
Published in The Astrophysical journal (20-12-2018)“…Because of their activity, late-type stars are known to host powerful flares producing intense high-energy radiation on short timescales that may significantly…”
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Influence of stellar radiation pressure on flow structure in the envelope of hot-Jupiter HD 209458b
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…Abstract Close-in exoplanets are subjected to extreme radiation of their host stars. Photometric observations of the hot-Jupiter HD 209458b transit by HST/STIS…”
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Structure of the circumbinary envelope around a young binary system
Published in Astronomy reports (01-12-2010)“…The structure of a circumstellar envelope around a young binary T Tauri star is considered. The supersonic orbital motion of the system components in the…”
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Reverse rotation of the accretion disk in RW Aur A: Observations and a physical model
Published in Astronomy reports (01-09-2012)“…Speckle interferometry of the young binary system RW Aur was performed with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy…”
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A possible mechanism for the formation of humps in the orbital light curves of WZ Sge cataclysmic variable stars
Published in Astronomy reports (01-03-2015)“…A mechanism for the formation of humps in the light curves of WZ Sge cataclysmic variables is proposed, based on the results of three-dimensional simulations…”
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NO Biomarker: Transmission and Emission Methods for Its Potential Detection in Exoplanet Atmospheres with Spektr-UF (WSO-UV)
Published in Astronomy reports (01-11-2023)“…Among all habitability factors for terrestrial exoplanets, one of the most important is the presence of a secondary N 2 –O 2 dominant atmosphere on an…”
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On Possible Types of Magnetospheres of Hot Jupiters
Published in Astronomy reports (01-07-2019)“…As a rule, the orbits of “hot Jupiter” exoplanets are located close to the Alfven point of the stellar wind of the host star. Many hot Jupiters could be in the…”
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Ionization fraction in the thermosphere of the exoplanet HD 209458b
Published in Solar system research (01-03-2014)“…Dissociation and ionization of hydrogen molecules and ionization of hydrogen atoms due to extreme UV radiation from the parent star are accompanied by the…”
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On the Possibility of Observing Nitric Oxide on Terrestrial Exoplanets Using the WSO-UV Observatory
Published in Astronomy reports (01-02-2023)“…It is generally believed that the presence of a -dominant atmosphere is an indication of biological and geological activity on terrestrial exoplanets that are…”
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Effect of the Orbit Eccentricity on the Flow in the Envelope of a Hot Jupiter
Published in Astronomy reports (01-11-2022)“…A three-dimensional numerical gas–dynamic model is presented. The aim of the model is to study the structure of the flow in the envelopes of hot Jupiters with…”
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Effect of Magnetic Field Diffusion on the Structure of Extended Envelopes of Hot Jupiters
Published in Astronomy reports (01-11-2022)“…The paper presents a modification of the numerical MHD model of extended envelopes of hot Jupiters, in which the magnetic viscosity is considered. In the new…”
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Symbiotic stars with spectral indication of bipolar ejection and stellar wind
Published in Astronomische Nachrichten (01-02-2014)“…Four out of a total of five symbiotic systems whose optical spectral lines contain satellite components indicating collimated ejection have an additional…”
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Self-Similar Perturbation of an Accretion Disc around Merging Black Holes
Published in Astronomy reports (01-11-2021)“…We study the possibility that merging of a binary black hole surrounded by a circumbinary accretion disc may produce an electromagnetic response. When black…”
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A Kinetic Model for Precipitation of Solar-Wind Protons into the Martian Atmosphere
Published in Astronomy reports (01-09-2021)“…— We present the kinetic Monte-Carlo model, which was developed to describe the influence of a proton flux from the undisturbed solar wind on the daytime…”
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Numerical Modeling of Mass Transfer in Close Binaries
Published in Astrophysics and space science (01-01-2005)“…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…”
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Possible New Envelope Types of Hot Jupiters
Published in Astronomy reports (01-07-2020)“…—For the case of the sub-Alfvén regime of the stellar wind flyby around the planet, the flow structure in the vicinity of a hot Jupiter have been studied by…”
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