activity
20012022
most citedVariable neutron star free precession in Hercules X-1 from evolution of RXTE X-ray pulse profiles with phase of the 35-day cycle

50 citations · 97 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2022★ 7 cited

On the appearance of non-local MRI in Keplerian accretion discs

Nikolay Shakura, Konstantin Postnov, Dmitry Kolesnikov +1

We revisit the modal analysis of small perturbations in Keplerian ideal gas flows leading to magneto-rotational instability (MRI) using the non-local approach. We consider the case…

astro-ph.HE2021★ 15 cited

Peculiar X-ray transient SRGA J043520.9+552226/AT2019wey discovered with SRG/ART-XC

I. A. Mereminskiy, A. V. Dodin, A. A. Lutovinov +24

Context: During the ongoing all-sky survey, the Mikhail Pavlinsky ART-XC telescope on board the SRG observatory should discover new X-ray sources, many of which can be transient. H…

astro-ph.HE2018★ 9 cited

Logarithmic potential for the gravitational field of Schwarzschild black holes

Nikolay I. Shakura, Galina V. Lipunova

Approximate gravitational potentials are often used to describe analytically the motion of particles near black holes (BHs), as well as to study the structure of an accretion disk.…

astro-ph.HE2017★ 9 cited

Wind Accretion - Observations Vs Theory

N. Shakura, K. Postnov

The theory of quasi-spherical subsonic accretion onto magnetized rotating neutron star is reviewed. Different regimes of quasi-spherical accretion onto a neutron star: supersonic (…

astro-ph.HE2014★ 1 cited

Origin of bright flares in SFXTs

K. Postnov, N. Shakura, L. Sidoli +1

In the settling accretion theory, which is applicable to quasi-spherical accreting slowly rotating magnetized neutron stars with X-ray luminosity ~erg/…

astro-ph.HE2013★ 50 cited

Variable neutron star free precession in Hercules X-1 from evolution of RXTE X-ray pulse profiles with phase of the 35-day cycle

K. Postnov, N. Shakura, . R. Staubert +3

Accretion of matter onto the surface of a freely precessing NS with a complex non-dipole magnetic field can explain the change of X-ray pulse profiles of Her X-1 observed by RXTE w…