Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Andrey Zhilkin"'
Publikováno v:
Galaxies, Vol 10, Iss 6, p 110 (2022)
A three-dimensional numerical model has been developed to study the flow structure in close binary systems with a magnetic field. The model uses a system of equations of modified magnetic hydrodynamics, which allows describing all the main dynamic ef
Externí odkaz:
https://doaj.org/article/fb1af8583e984292ba86e8b2832b24ae
Publikováno v:
Galaxies, Vol 9, Iss 4, p 110 (2021)
In this paper, the characteristics of hot spots on an accretor surface are investigated for two types of polars: the eclipsing synchronous polar V808 Aur and the non-eclipsing asynchronous polar CD Ind in configuration of an offset and non-offset mag
Externí odkaz:
https://doaj.org/article/0648c46b4c394655a6ae4e9d34ea6500
Autor:
Andrey Zhilkin, Dmitri Bisikalo
Publikováno v:
Universe, Vol 7, Iss 11, p 422 (2021)
A numerical model description of a hot Jupiter extended envelope based on the approximation of multi-component magnetic hydrodynamics is presented. The main attention is focused on the problem of implementing the completed MHD stellar wind model. As
Externí odkaz:
https://doaj.org/article/88e357a64e5240ec90c3e1f514178cc1
Publikováno v:
Astronomy Reports. 65:676-692
Most hot Jupiters have extended envelopes of gas that spread beyond their Roche lobes. A typical envelope is weakly gravitationally bound to the planet and, therefore, its structure and properties are strongly affected by stellar wind disturbances, f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b641d6be994c3c80883fa56d220e4048
https://doi.org/10.1134/s1063772921090092
https://doi.org/10.1134/s1063772921090092
Publikováno v:
Astronomy Reports. 65:392-411
We performed a three-dimensional numerical MHD simulation of the flow structure in the asynchronous polar CD Ind during the switching phases between the magnetic poles of the accretor—a white dwarf. To account for fast processes, a numerical non-st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1a0b0114066cb0a82fec1c0d9adfe21e
https://doi.org/10.1134/s106377292106007x
https://doi.org/10.1134/s106377292106007x
Publikováno v:
Astronomy Reports. 65:203-208
This paper presents the results of calculating the efficiency of solar wind proton charge exchange as a function of variations in the column density of hydrogen atoms in the extended corona of Mars. The presence of regular density variations has been
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::99d408ea243f73b940acb3f1093fbc25
https://doi.org/10.1134/s1063772921030033
https://doi.org/10.1134/s1063772921030033
Autor:
D. V. Bisikalo, Andrey Zhilkin
Publikováno v:
Astronomy Reports. 64:563-577
—For the case of the sub-Alfven regime of the stellar wind flyby around the planet, the flow structure in the vicinity of a hot Jupiter have been studied by three-dimensional numerical simulation. As an example, the hot Jupiter HD 209458b was consi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9b587d6320e4296cbf203db0eb2572e0
https://doi.org/10.1134/s1063772920080090
https://doi.org/10.1134/s1063772920080090
Publikováno v:
Astronomy Reports. 64:467-498
The flow structure in the asynchronous polar CD Ind was investigated in the approximation of an offset dipole. Computation results made it possible to identify such system features as the drift of hot spots over the white dwarf surface, the flow stru
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::20cc9b74094e9cc5388d71c68d7c621a
https://doi.org/10.1134/s1063772920070069
https://doi.org/10.1134/s1063772920070069
Publikováno v:
Proceedings of the International Astronomical Union. 16:228-233
In this paper, the effect of hot spots movement by accretor surface on the appearance of bolometric light curves for two types of polars - synchronous V808 Aur and asynchronous CD Ind is studied. The analysis was carried out under the assumption of a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5579e924e73806cdb5b5e691bfe81a44
https://doi.org/10.1017/s1743921322001417
https://doi.org/10.1017/s1743921322001417
Autor:
Sergey Khaibrakhmanov, Sergey Zamozdra, Natalya Kargaltseva, Andrey Zhilkin, Alexander Dudorov
Publikováno v:
Proceedings of the International Astronomical Union. 16:273-278
We numerically investigate the gravitational collapse of rotating magnetic protostellar clouds. The simulations are performed using 2D MHD code ‘Enlil’. The code is based on TVD scheme of increased order of accuracy. We developed a model of the i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5e3b52f5674b545cfe26f7e578f72782
https://doi.org/10.1017/s1743921322001302
https://doi.org/10.1017/s1743921322001302