activity
20012025
most citedOn the mass transfer in AE Aquarii

32 citations · 161 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.HE2025★ 1 cited

MAD-Accretion Scenario in High-Mass X-Ray Binaries with Neutron Stars

N. R. Ikhsanov, M. Yu. Piotrovich, N. G. Beskrovnaya

The wind-fed accretion of gas with an intrinsic magnetic field onto neutron stars in high-mass X-ray binaries (HMXBs) is discussed. The criteria for the implementation of quasi-sph…

astro-ph.HE2025★ 1 cited

Stellar wind parameters of massive stars in accretion-powered High Mass X-ray Binary Pulsars

N. Beskrovnaya, N. Ikhsanov, V. Kim

The process of mass-exchange between the components of High Mass X-ray Binary (HMXB) systems with neutron stars undergoing wind-fed accretion is discussed. The X-ray luminosity of…

astro-ph.SR2017★ 5 cited

Magnetic field and radial velocities of the star Chi Draconis A

Byeong-Cheol Lee, D. Gadelshin, Inwoo Han +13

We present high-resolution spectropolarimetric observations of the spectroscopic binary Chi Dra. Spectral lines in the spectrum of the main component Chi Dra A show variable Zeeman…

astro-ph.HE2016★ 2 cited

AR Scorpii is a new white dwarf in the ejector state

N. G. Beskrovnaya, N. R. Ikhsanov

Marsh et al. (2016) have recently reported the discovery of a radio-pulsing white dwarf in the cataclysmic variable AR Sco. The period of pulsations which are also seen in the opti…

astro-ph.SR2016★ 13 cited

Features of the Matter Flows in the Peculiar Cataclysmic Variable AE Aquarii

P. B. Isakova, N. R. Ikhsanov, A. G. Zhilkin +2

The structure of plasma flows in close binary systems in which one of the components is a rapidly rotating magnetic white dwarf is studied. The main example considered is the AE Aq…

astro-ph.HE2014★ 5 cited

A scenario of the formation of isolated X-ray pulsars with anomalously long period

N. R. Ikhsanov, V. Yu. Kim, N. G. Beskrovnaya

A scenario of the formation of isolated X-ray pulsars is discussed with an application to one of the best studied objects of this class 1E 161348-5055. This moderately luminous, 10…