activity
19982019
most citedDiscrete sources as the origin of the Galactic X-ray ridge emission

234 citations · 3.8k across the 87 of their papers we have counts for

collaborators

88 papers

astro-ph.SR2019★ 8 cited

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…

astro-ph.HE2017

Modeling of High-Frequency Variability in X-ray Binaries with Black Holes

A. N. Semena, M. G. Revnivtsev, T. I. Larchenkova +1

The properties of the aperiodic variability in X-ray binaries with black holes are considered. The power spectra of the luminosity variability for a flat accretion disk that is an…

astro-ph.HE2017★ 7 cited

Sample of Cataclysmic Variables from 400d X-ray Survey

R. A. Burenin, M. G. Revnivtsev, A. Yu. Tkachenko +6

We present a sample of cataclysmic variables (CVs) identified among the X-ray sources from the 400 square degree X-ray survey based on ROSAT pointing data (400d). The procedure of…

astro-ph.HE2016

Sample of Cataclysmic Variables from 400d X-ray Survey

R. Burenin, M. Revnivtsev, A. Tkachenko +6

We present a sample of eight cataclysmic variables (CVs) identified among the X-ray sources of the 400 square degree (400d) X-ray ROSAT/PSPC survey. Based on this sample, we have o…

astro-ph.HE2016★ 56 cited

The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

Valery F. Suleimanov, Juri Poutanen, Joonas Nättilä +3

Determining neutron star (NS) radii and masses can help to understand the properties of matter at supra-nuclear densities. Thermal emission during thermonuclear X-ray bursts from N…

astro-ph.HE2016★ 18 cited

Observations of the X-ray pulsar LMC X-4 with NuSTAR: limit on the magnetic field and tomography of the system in the fluorescent iron line

A. E. Shtykovsky, A. A. Lutovinov, V. A. Arefiev +2

We present results of the spectral and timing analysis of the X-ray pulsar LMC X-4 with the NuSTAR observatory in the broad energy range 3-79 keV. Along with the detailed analysis…