activity
20152025
most citedOn the dependence of the X-ray continuum variations with luminosity in accreting X-ray pulsars

76 citations · 323 across the 9 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2025★ 1 cited

Radiation-dominated polar emitting region of an accreting X-ray pulsar -- I. Polarization- and spectrum-dependent structure, and the emergent continuum

M. I. Gornostaev

The radiation-dominated polar emitting region of an accreting X-ray pulsar is simulated numerically in the framework of a three-dimensional (geometrically two-dimensional) model. T…

astro-ph.HE2022

On thermalization of radiation in hydrostatic atmospheres

M. I. Gornostaev

The problem of thermalization of radiation within a self-emitting hydrogen isothermal atmosphere is considered for the case of a hydrostatic profile of the plasma density. The prob…

astro-ph.HE2021★ 46 cited

X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum

E. Sokolova-Lapa, M. Gornostaev, J. Wilms +12

Recent observations of X-ray pulsars at low luminosities allow, for the first time, to compare theoretical models for the emission from highly magnetized neutron star atmospheres a…

astro-ph.HE2020★ 14 cited

Three-dimensional modelling of accretion columns: spatial asymmetry and self-consistent simulations

M. I. Gornostaev

The paper presents the results of three-dimensional (3D) modelling of the structure and the emission of accretion columns formed above the surface of accreting strongly magnetized…

astro-ph.CO2020

Comptonization of CMB in galaxy clusters. Monte Carlo computations

M. I. Gornostaev, G. V. Lipunova

The problem under consideration is to determine the change of the Cosmic Microwave Background (CMB) spectral shape due to the thermal Sunyaev-Zeldovich effect. We numerically model…

astro-ph.HE2017★ 60 cited

Luminosity-dependent changes of the cyclotron line energy and spectral hardness in Cep X-4

V. Vybornov, D. Klochkov, M. Gornostaev +5

X-ray spectra of accreting pulsars are generally observed to vary with their X-ray luminosity. In particular, the hardness of the X-ray continuum is found to depend on luminosity.…

astro-ph.HE2016★ 50 cited

Discovery and Modeling of a Flattening of the Positive Cyclotron Line/Luminosity Relation in GX 304-1 with RXTE

Richard E. Rothschild, Matthias Kuehnel, Katja Pottschmidt +8

The RXTE observed four outbursts of the accreting X-ray binary transient source, GX 304-1 in 2010 and 2011. We present results of detailed 3-100 keV spectral analysis of 69 separat…

astro-ph.HE2015★ 76 cited

On the dependence of the X-ray continuum variations with luminosity in accreting X-ray pulsars

K. A. Postnov, M. I. Gornostaev, D. Klochkov +3

Using RXTE/ASM archival data, we investigate the behaviour of the spectral hardness ratio as a function of X-ray luminosity in a sample of six transient X-ray pulsars (EXO 2030+375…