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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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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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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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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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Model-independent restoration of the brightness distribution across the disks of stars from high precision eclipsing light curves.
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- Astrophysics, 2008, v. 51, n. 4, p. 506, doi. 10.1007/s10511-008-9038-0
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Evolution of the components of the close binary WR 20a.
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- Astronomy Reports, 2008, v. 52, n. 8, p. 656, doi. 10.1134/S1063772908080064
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Search for exotic matter from gravitational microlensing observations of stars.
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- Astrophysics & Space Science, 2008, v. 317, n. 3/4, p. 181, doi. 10.1007/s10509-008-9870-z
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Spectroscopic monitoring of SS 433: A search for long-term variations of kinematic model parameters.
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- Astronomy Reports, 2008, v. 52, n. 6, p. 487, doi. 10.1134/S1063772908060061
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The mass of the compact object in the X-ray binary her X-1/HZ her.
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- Astronomy Reports, 2008, v. 52, n. 5, p. 379, doi. 10.1134/S1063772908050041
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Synthesis of Line Profiles and Radial Velocity Curves for X-Ray Binary Systems.
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- Astrophysics & Space Science, 2006, v. 304, n. 1-4, p. 263, doi. 10.1007/s10509-006-9126-8
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The mass of the compact object in the low-mass X-ray binary 2S 0921-630.
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- Astronomy Reports, 2006, v. 50, n. 7, p. 544, doi. 10.1134/S1063772906070043
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Dependence of the Absorption-Line Profiles and Radial-Velocity Curve of the Optical Star in an X-ray Binary on the Orbital Inclination and Component-Mass Ratio.
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- Astronomy Reports, 2005, v. 49, n. 10, p. 801, doi. 10.1134/1.2085250
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Supermassive Black Holes: Relation to Dark Halos.
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- Astronomy Reports, 2005, v. 49, n. 5, p. 362, doi. 10.1134/1.1923545
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Evolution of the Masses of Neutron Stars in Binary Systems.
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- Astronomy Reports, 2005, v. 49, n. 4, p. 295, doi. 10.1134/1.1898407
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Interpretation of the Light Curves of “Quiescent” X-Ray Novae in a Model with a Noncollisional Interaction between the Flow and Disk. The XTE J1118+480 System.
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- Astronomy Reports, 2005, v. 49, n. 2, p. 79, doi. 10.1134/1.1862355
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Gravitational Darkening Coefficients of the Stars in the Semidetached Binary V Puppis.
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- Astronomy Reports, 2005, v. 49, n. 2, p. 102, doi. 10.1134/1.1862357
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Radial-Velocity Curves and Theoretical Spectral-Line Profiles of the Components of Low-Mass Close X-ray Binary Systems.
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- Astronomy Reports, 2005, v. 49, n. 2, p. 109, doi. 10.1134/1.1862358
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Parameters of V404 Cyg—A Black-Hole Binary.
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- Astronomy Reports, 2004, v. 48, n. 12, p. 1019, doi. 10.1134/1.1836025
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A Hard X-ray Survey of the Sagittarius Arm Tangent with the IBIS Telescope of the INTEGRAL Observatory: A Catalog of Sources.
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- Astronomy Letters, 2004, v. 30, n. 8, p. 534, doi. 10.1134/1.1784495
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Estimate of the Black-Hole Mass and Orbital Inclination from the Radial-Velocity Curve of the X-Ray Binary Cyg X-1.
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- Astronomy Reports, 2004, v. 48, n. 7, p. 550, doi. 10.1134/1.1777273
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Masses of X-ray Pulsars in Binary Systems with OB Supergiants.
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- Astronomy Reports, 2004, v. 48, n. 2, p. 89, doi. 10.1134/1.1648072
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Massive Close Binary Stars and Gamma-ray Bursts.
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- Astronomy Reports, 2004, v. 48, n. 1, p. 39, doi. 10.1134/1.1641121
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Masses of Stellar Black Holes and Testing Theories of Gravitation.
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- Astronomy Reports, 2003, v. 47, n. 12, p. 989, doi. 10.1134/1.1633612
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Light Curve Interpretation for “Quiescent” X- ray Novae in a Model with Noncollisional Interaction Between the Flow and Disk. The System GU Mus = GRS 1124–68.
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- Astronomy Reports, 2003, v. 47, n. 8, p. 621, doi. 10.1134/1.1601631
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Wolf–Rayet Stars, Black Holes, and Gamma-Ray Bursters in Close Binaries.
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- Astronomy Reports, 2003, v. 47, n. 5, p. 386, doi. 10.1134/1.1575853
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Interpretation of Light Curves of the Cataclysmic Variable OY Car in a Model with Shockless Interaction between a Gaseous Stream and the Disk.
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- Astronomy Reports, 2003, v. 47, n. 3, p. 214, doi. 10.1134/1.1562216
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The Evolution of GRS 1915+105—an X-ray Binary with a Black Hole.
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- Astronomy Reports, 2003, v. 47, n. 1, p. 20, doi. 10.1134/1.1538493
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Evolution of Wolf–Rayet Stars in Binary Systems: An Analysis of the Mass and Orbital-Eccentricity Distributions.
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- Astronomy Reports, 2003, v. 47, n. 1, p. 38, doi. 10.1134/1.1538495
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