activity
20132025
most citedSupercritical Accretion Discs in Ultraluminous X-ray Sources and SS 433

113 citations · 418 across the 29 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 2 cited

NGC 5474 X-1: a neutron star ULX in an old stellar cluster?

Kirill Atapin, Alexander Vinokurov, Arkadiy Sarkisyan +4

We present the optical and X-ray study of the ultraluminous X-ray source (ULX) NGC 5474 X-1. The X-ray spectrum taken during the bright state of the source ($L_X \sim 2\times10^{40…

astro-ph.HE2020★ 1 cited

Determining parameters of ULXs with model grids of extended atmospheres

A. Kostenkov, A. Vinokurov, Y. Solovyeva

In current work we continued study of wind parameters of ultraluminous X-ray sources (ULXs) using model grids of extended atmospheres. We present sets of models with temperatures f…

astro-ph.HE2020★ 4 cited

Observations of ultraluminous X-ray sources with the 6-m telescope of the SAO RAS

A. Vinokurov, K. Atapin, Y. Solovyeva +2

The nature of ultraluminous X-ray sources (ULXs) is not yet fully understood but it can be done in the most efficient way by analyzing its optical emission and environment. We pres…

astro-ph.SR2020★ 9 cited

Luminous Blue Variable candidates in M31

A. Sarkisyan, O. Sholukhova, S. Fabrika +7

We study five Luminous Blue Variable (LBV) candidates in the Andromeda galaxy and one more (MN112) in the Milky Way. We obtain the same-epoch near-infrared (NIR) and optical spectr…

astro-ph.SR2020★ 11 cited

New luminous blue variable candidates in the NGC 247 galaxy

Y. Solovyeva, A. Vinokurov, A. Sarkisyan +6

We search for LBV stars in galaxies outside the Local Group. Here we present a study of two bright sources in the NGC 247 galaxy. Object j004703.27-204708.4 ($M_V=-9.08 \pm 0.…

astro-ph.HE2020★ 10 cited

Modeling of extended atmospheres with temperatures below 40000K

A. Kostenkov, A. Vinokurov, Y. Solovyeva +2

We calculate models of extended stellar atmospheres with a temperature in the range of 12000-40000K and a mass loss rate of yr. A large number of…