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20042025
most citedThe Mass of the Compact Object in the X-Ray Binary Her X-1/HZ Her

165 citations · 494 across the 21 of their papers we have counts for

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10 papers · 1 filter

astro-ph.SR2025

The massive binary system WR 20a: light curve analysis in a colliding wind model

I. I. Antokhin, E. A. Antokhina, A. M. Cherepashchuk

The article presents the results of the analysis of optical light curves of the massive binary system WR 20a (WN 6ha + WN 6ha). The analysis was performed with the binary system mo…

astro-ph.SR2021★ 8 cited

On the nature of the single eclipse per 80d orbit of the H-rich luminous WN star WR22

Guillaume Lenoir-Craig, Igor I. Antokhin, Eleonora A. Antokhina +2

WR22 = HD 92740 is a bright (V = 6.4 ), intrinsically luminous, double-line WN7h + O9III-V binary exhibiting one sharp 8\% deep eclipse near periastron in its elliptical (e =…

astro-ph.SR2020★ 14 cited

Discovery of a pre-cataclysmic binary with unusual chromaticity of the eclipsed white dwarf by the GPX Survey

Vadim Krushinsky, Paul Benni, Artem Burdanov +14

We report the discovery of a relatively bright eclipsing binary system, which consists of a white dwarf and a main sequence K7 star with clear signs of chromospheric and spot activ…

astro-ph.SR2017★ 7 cited

Masses of optical components and black holes in x-ray novae: the effects of components proximity

V. S. Petrov, E. A. Antokhina, A. M. Cherepashchuk

An exact calculation of CaI A absorption profiles in the spectra of optical stars in low-mass X-ray binary systems with black holes (BH LMXBs) is carried out. We show th…

astro-ph.SR2016

Accuracy of the component mass estimation methods in LMXB

E. A. Antokhina, V. S. Petrov, A. M. Cherepashchuk

There is a mismatch between modelled and observed distributions of optical stars masses in BH LMXB. Companion masses in BH LMXB are found in the mass range 0.1 - 1.6 wi…

astro-ph.SR2013★ 10 cited

The K-corrections to radial velocity curves of optical components in X-Ray Binaries. HMXB with weak X-ray heating

V. S. Petrov, E. A. Antokhina, A. M. Cherepashchuk

The radial velocity curves of optical components in X-ray binary systems can differ from the radial velocity curves of their barycenters due to tidal distortion, gravitational dark…

astro-ph.SR2012★ 165 cited

The Mass of the Compact Object in the X-Ray Binary Her X-1/HZ Her

M. K. Abubekerov, E. A. Antokhina, A. M. Cherepashchuk +1

We have obtained the first estimates of the masses of the components of the Her X-1/HZ Her X-ray binary system taking into account non-LTE effects in the formation of the H_gamma a…

astro-ph.SR2012★ 13 cited

The Mass of the Compact Object in the Low-Mass X-ray Binary 2S 0921-630

M. K. Abubekerov, E. A. Antokhina, A. M. Cherepashchuk +1

We interpret the observed radial-velocity curve of the optical star in the low-mass X-ray binary 2S 0921-630 using a Roche model, taking into account the X-ray heating of the optic…

astro-ph.SR2010★ 7 cited

Light Curve Analysis of Hipparcos Data for the Massive O-type Eclipsing Binary UW CMa

E. A. Antokhina, M. Srinivasa Rao, M. Parthasarathy

Hipparcos photometric data for the massive O-type binary UW CMa were analysed within the framework of the Roche model. Photometric solutions were obtained for five mass ratios in t…

astro-ph.SR2009★ 24 cited

The Mass of the Black Hole in the X-ray Binary M33 X-7 and the Evolutionary Status of M33 X-7 and IC 10 X-1

M. K. Abubekerov, E. A. Antokhina, A. I. Bogomazov +1

We have analyzed the observed radial-velocity curve for the X-ray binary M33 X-7 in a Roche model. We have analyzed the dependence between the component masses and the degree of fi…