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On the Possibility to Estimate the Orbital Eccentricity of a Binary System with an Exoplanet from a Transit Light Curve.
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- Astronomy Reports, 2023, v. 67, n. 11, p. 1096, doi. 10.1134/S106377292311001X
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X-Ray Astronomy and Close Binary Systems.
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- Astronomy Reports, 2023, v. 67, n. 9, p. 856, doi. 10.1134/S1063772923090020
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Observations of X-ray Binaries at the Caucasus Mountain Observatory of SAI MSU.
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- Astrophysical Bulletin, 2023, v. 78, n. 3, p. 259, doi. 10.1134/S1990341323700062
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New Forms of Matter in the Universe.
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- Astronomy Reports, 2023, v. 67, n. 8, p. 790, doi. 10.1134/S1063772923080036
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Effect of the Eccentricity of the Planet's Orbit on the Limb Darkening Coefficients of the Eclipsed Star.
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- Astronomy Reports, 2023, v. 67, n. 2, p. 151, doi. 10.1134/S1063772923020026
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Optical Monitoring of SS 433 in 2017–2021.
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- Astronomy Reports, 2022, v. 66, n. 6, p. 451, doi. 10.1134/S1063772922060026
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Parameters of X-Ray Binary Sco X-1 in the Model of Partial Filling of Roche Lobe by Optical Star.
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- Astronomy Reports, 2022, v. 66, n. 4, p. 348, doi. 10.1134/S1063772922040023
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Close Binary Stars. I: Simple Models.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S5, doi. 10.1134/S1063772922130030
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Close Binary Stars. II: Parametric Models in Inverse Problems of Astrophysics.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S70, doi. 10.1134/S1063772922130042
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Close Binary Stars. III: Roche Model.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S123, doi. 10.1134/S1063772922130054
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Close Binary Stars. IV: Applications of the Roche Model.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S168, doi. 10.1134/S1063772922130066
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Close Binary Stars. V: Eclipsing Star Systems with Extended Atmospheres.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S348, doi. 10.1134/S1063772922130078
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Close Binary Stars. VI: New Research Methods.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S412, doi. 10.1134/S106377292213008X
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Close Binary Stars. VII: On the Evolution of Close Binary Systems.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S498, doi. 10.1134/S1063772922130091
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Close Binary Stars. VIII: Close Binary Star Systems in the Late Stages of Evolution.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S567, doi. 10.1134/S1063772922130108
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Close Binary Stars. IX: Statistical Studies of Close Binary Systems.
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- Astronomy Reports, 2022, v. 66, n. 2, p. S692, doi. 10.1134/S106377292213011X
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Progress in Understanding the Nature of SS433.
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- Universe (2218-1997), 2022, v. 8, n. 1, p. 13, doi. 10.3390/universe8010013
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Optical Spectroscopy of Quasars Discovered by SRG/eROSITA with a 2.5-m Telescope at the Caucasus Mountain Observatory of SAI MSU.
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- Astronomy Letters, 2021, v. 47, n. 10, p. 661, doi. 10.1134/S1063773721100029
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Investigation of Spectral Characteristics and Statistical Properties of Flicker Noise of the X-Ray Nova A0620-00.
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- Astronomy Reports, 2021, v. 65, n. 9, p. 839, doi. 10.1134/S1063772921090067
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Transient Double-Beam Spectrograph for the 2.5-m Telescope of the Caucasus Mountain Observatory of SAI MSU.
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- Astronomy Letters, 2020, v. 46, n. 12, p. 836, doi. 10.1134/S1063773720120038
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Spectroscopic Monitoring of SS 433. Stability of Parameters of the Kinematic Model over 40 Years.
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- Astronomy Reports, 2018, v. 62, n. 11, p. 747, doi. 10.1134/S106377291811001X
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WR + OB Binary Systems: Observational Evidence of Their Formation as a Result of Mass Exchange.
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- Astronomy Reports, 2018, v. 62, n. 9, p. 567, doi. 10.1134/S1063772918090032
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Formation of close binary black holes merging due to gravitational-wave radiation.
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- Astronomy Reports, 2017, v. 61, n. 10, p. 833, doi. 10.1134/S1063772917100092
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ASTRONIRCAM-the infrared camera-spectrograph for the 2.5-m telescope of SAI Caucasian observatory.
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- Astrophysical Bulletin, 2017, v. 72, n. 3, p. 349, doi. 10.1134/S1990341317030245
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Masses of the visual components and black holes in X-ray novae: Effects of proximity of the components.
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- Astronomy Reports, 2017, v. 61, n. 5, p. 377, doi. 10.1134/S106377291705002X
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Black holes in close binary systems and galactic nuclei.
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- Astronomy Reports, 2017, v. 61, n. 4, p. 265, doi. 10.1134/S1063772917040035
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Coronagraphic methods for detecting faint astronomical objects near bright ones: Application to the 2.5-m telescope of Sternberg Astronomical Institute.
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- Astronomy Reports, 2017, v. 61, n. 3, p. 169, doi. 10.1134/S1063772917030039
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Estimation of the accuracy of methods for determining component masses for low-mass X-ray binary systems.
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- Astronomy Reports, 2017, v. 61, n. 1, p. 1, doi. 10.1134/S1063772917010012
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The mass of the black hole in the X-ray binary LMC X-1.
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- Astronomy Reports, 2016, v. 60, n. 12, p. 1029, doi. 10.1134/S1063772916120015
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The evolution of close binary stars.
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- Astronomy Reports, 2016, v. 60, n. 5, p. 461, doi. 10.1134/S1063772916050024
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RESOLVED PHOTOMETRY OF THE BINARY COMPONENTS OF RW Aur.
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- Information Bulletin on Variable Stars, 2015, n. 6145, p. 1
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Taking into account the effects of component proximity on the spectral-line profiles of stars in low-mass X-ray binary systems.
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- Astronomy Reports, 2015, v. 59, n. 5, p. 346, doi. 10.1134/S1063772915050066
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RESOLVED PHOTOMETRY OF THE BINARY COMPONENTS OF RW Aur.
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- Information Bulletin on Variable Stars, 2015, n. 6126, p. 1
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Limb-darkening anomalies in stars eclipsed by exoplanets.
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- Astronomy Reports, 2015, v. 59, n. 1, p. 1, doi. 10.1134/S1063772915010011
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Stability of the parameters of the Stellar black-hole mass distribution estimated using nonparametric methods.
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- Astronomy Reports, 2014, v. 58, n. 3, p. 113, doi. 10.1134/S1063772914030068
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Supermassive black holes and central star clusters: Connection with the host galaxy kinematics and color.
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- Astronomy Reports, 2013, v. 57, n. 11, p. 797, doi. 10.1134/S1063772913110085
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Compact nuclear objects and properties of their parent galaxies.
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- Proceedings of the International Astronomical Union, 2013, v. 9, n. S304, p. 379, doi. 10.1017/S1743921314004359
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Wolf-Rayet stars with relativistic companions.
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- Astronomy Reports, 2013, v. 57, n. 9, p. 657, doi. 10.1134/S1063772913090084
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<i>K</i>-Corrections to radial-velocity curves of optical components in X-ray binaries. Massive systems with weak X-ray heating.
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- Astronomy Reports, 2013, v. 57, n. 9, p. 669, doi. 10.1134/S1063772913090047
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Spectral and photometric studies of the Wolf-Rayet star WR 134 = HD 191765.
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- Astronomy Reports, 2012, v. 56, n. 10, p. 761, doi. 10.1134/S1063772912100058
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Analysis of light curves of eclipsing systems with exoplanets: HD 189733.
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- Astronomy Reports, 2011, v. 55, n. 12, p. 1051, doi. 10.1134/S1063772911120018
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Supermassive black holes and galaxy kinematics.
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- Astronomy Reports, 2011, v. 55, n. 7, p. 595, doi. 10.1134/S1063772911070109
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The Wolf-Rayet star HD 192163 as a possible evolutionary progenitor of a low-mass X-ray binary.
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- Astronomy Reports, 2011, v. 55, n. 4, p. 347, doi. 10.1134/S1063772911010069
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The evolutionary status of the most massive WNh stars in close binary systems. NGC 3603-A1.
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- Astronomy Reports, 2011, v. 55, n. 3, p. 247, doi. 10.1134/S1063772911030085
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Light curve analysis for eclipsing systems with exoplanets. The system HD 209458.
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- Astronomy Reports, 2010, v. 54, n. 12, p. 1105, doi. 10.1134/S1063772910120048
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Jumber Georgievich Lominadze (In honor of his 80th birthday).
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- Plasma Physics Reports, 2010, v. 36, n. 9, p. 824, doi. 10.1134/S1063780X10090102
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Kinematics of disk galaxies with known masses of their supermassive black holes. Observations.
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- Astronomy Reports, 2010, v. 54, n. 7, p. 578, doi. 10.1134/S1063772910070024
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Estimation of parameter errors in inverse problems. Determining limb-darkening coefficients in classical eclipsing systems.
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- Astronomy Reports, 2009, v. 53, n. 8, p. 722, doi. 10.1134/S1063772909080046
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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.
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- Astronomy Reports, 2009, v. 53, n. 3, p. 232, doi. 10.1134/S1063772909030056
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Population synthesis for massive close WR20a-type binaries.
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- Astronomy Reports, 2008, v. 52, n. 12, p. 1009, doi. 10.1134/S1063772908120068
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