32 citations · 146 across the 18 of their papers we have counts for
17 papers
Primary disks and their observational appearance in collapsing magnetic rotating protostellar clouds
Natalya S. Kargaltseva, Sergey A. Khaibrakhmanov, Alexander E. Dudorov +1
The collapse of the magnetic rotating protostellar cloud with mass of is numerically studied. The initial ratios of the thermal, magnetic, and rotational energies o…
Influence of the magnetic field on the formation of protostellar disks
N. S. Kargaltseva, S. A. Khaibrakhmanov, A. E. Dudorov +2
We numerically model the collapse of magnetic rotating protostellar clouds with mass of 10 . The simulations are carried out with the help of 2D MHD code Enlil. The struct…
Features of the Accretion in the EX Hydrae System: Results of Numerical Simulation
P. B. Isakova, A. G. Zhilkin, D. V. Bisikalo +2
A two dimensional numerical model in the axisymmetric approximation that describes the flow structure in the magnetosphere of the white dwarf in the EX Hya system has been develope…
Features of the Flow Structure in the Vicinity of the Inner Lagrangian Point in Polars
P. B. Isakova, A. G. Zhilkin, D. V. Bisikalo
The structures of plasma flows in close binary systems whose accretors have strong intrinsic magnetic fields are studied. A close binary system with the parameters of a typical pol…
On one effect of coronal mass ejections influence on the envelopes of hot Jupiters
A. G. Zhilkin, D. V. Bisikalo, P. V. Kaigorodov
It is now established that the hot Jupiters have extensive gaseous (ionospheric) envelopes, which expanding far beyond the Roche lobe. The envelopes are weakly bound to the planet…
On possible types of magnetospheres of hot Jupiters
A. G. Zhilkin, D. V. Bisikalo
We show that the orbits of exoplanets of the "hot Jupiter" type, as a rule, are located close to the Alfven point of the stellar wind of the parent star. At this, many hot Jupiters…