activity
20052023
most citedOn the possible electromagnetic manifestations of merging black holes

7 citations · 13 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2023

Turbulent convection in protoplanetary discs and its role in angular momentum transfer

E. P. Kurbatov, Ya. N. Pavlyuchenkov

We present a model for the transport of anisotropic turbulence in an accretion disc. The model uses the Reynolds stress tensor approach in the mean field approximation. To study th…

astro-ph.EP2021★ 1 cited

The role of atmospheric outflows in the migration of hot Jupiters

Evgeny P. Kurbatov, Dmitri V. Bisikalo

Many of observed hot Jupiters are subject to atmospheric outflows. Numerical simulations have shown that the matter escaping from the atmosphere can accumulate outside the orbit of…

astro-ph.HE2018★ 7 cited

On the possible electromagnetic manifestations of merging black holes

D. V. Bisikalo, A. G. Zhilkin, E. P. Kurbatov

We consider scenario of merger of two stellar mass black holes surrounded by an accretion disk. Due to emission of gravitational waves, the mass of the central object decreases and…

astro-ph.SR2018

On the possible mechanism of radio emission of polars

E. P. Kurbatov, A. G. Zhilkin, D. V. Bisikalo

We suggest a mechanism for generation of radio emission from polars. It is based on the cyclotron radiation of thermal electrons at the background of fluctuating magnetic field. Th…

astro-ph.SR2017★ 4 cited

Excitation of turbulence in accretion disks of binary stars by non-linear perturbations

E. P. Kurbatov, D. V. Bisikalo

Accretion disks in binary systems can experience hydrodynamic impact at inner as well as outer edges. The first case is typical for protoplanetary disks around young T Tau stars. T…

astro-ph.IM2016

On the technique for the recovery of the spectrum of turbulence in astrophysical disks

D. V. Bisikalo, E. P. Kurbatov, Ya. N. Pavlyuchenkov +2

We present a method that can be used to recover the spectrum of turbulence from observations of optically thin emission lines formed in astrophysical disks. Within this method we a…