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Parameters of the X-ray binary system Scorpius X-1

Monthly notices of the Royal Astronomical Society, 2021-11, Vol.508 (1), p.1389-1403

2021

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Optical, J and K light curves of XTE J1118+480 = KV UMa: the mass of the black hole and the spectrum of the non-stellar component

Monthly notices of the Royal Astronomical Society, 2019-12, Vol.490 (3), p.3287-3308

2019

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I -band photometry of the quiescent black hole X-ray nova GROJ0422 + 32 = V518 Per: modelling of the orbital light curve and estimation of the black hole mass

Monthly notices of the Royal Astronomical Society, 2024-06, Vol.531 (4), p.4917-4928

2024

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Population synthesis of AX J1745.6−2901 X-ray nova-type binaries with rapidly decreasing orbital periods

Monthly notices of the Royal Astronomical Society, 2022-07, Vol.514 (4), p.5375-5384

2022

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Study of the Rapid Variability of a Dwarf Nova SS Cyg at Different Brightness Levels

Astronomy reports, 2024-02, Vol.68 (2), p.129-160

2024

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Optical and J, K -photometry of the quiescent black hole X-ray nova A0620−00 in the passive and active states

Monthly notices of the Royal Astronomical Society, 2019-02, Vol.483 (1), p.1067-1079

2019

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Parameters of X-Ray Binary Sco X-1 in the Model of Partial Filling of Roche Lobe by Optical Star

Astronomy reports, 2022, Vol.66 (4), p.348-358

2022

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Parameter Determination for the Eclipsing Long-Period Dwarf Nova EX Dra from Photometric Observations during Different Activity States of the System

Astronomy reports, 2019-07, Vol.63 (7), p.571-594

2019

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Analysis of Photometric Observations of the New Cataclysmic Variable ASASSN-13cx

Astronomy reports, 2018, Vol.62 (1), p.31-49

2018

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Photometric behavior of the cataclysmic variable SDSS J150240.98+333423.9/NZ Boo in quiescence

Astronomy reports, 2015-05, Vol.59 (5), p.366-384

2015

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Light-curve syntheses for close binary systems: Modeling spiral waves in an elliptical disk around a white dwarf

Astronomy reports, 2005-10, Vol.49 (10), p.783-800

Khruzina, T S

2005

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Structure of the accretion disk in the cataclysmic variable UX uma in the transition to its quiescent state

Astronomy reports, 2007-04, Vol.51 (4), p.318-338

2007

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The dwarf nova V1239 herculis in quiescence

Astronomy reports, 2015-04, Vol.59 (4), p.288-312

2015

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Light-curve synthesis for close binaries: An extended shock as an analog of a hot spot in cataclysmic variables

Astronomy reports, 2001-04, Vol.45 (4), p.255-268

Khruzina, T S

2001

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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

Astronomy reports, 2005-02, Vol.49 (2), p.79-88

2005

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Light-curve synthesis for close binaries: Elliptical disk around a white dwarf

Astronomy reports, 2000-07, Vol.44 (7), p.446-459

Khruzina, T S

2000

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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

Astronomy reports, 2003-03, Vol.47 (3), p.214-231

2003

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Interpretation of orbital light curves of U Geminorum

Astronomy reports, 2003-10, Vol.47 (10), p.848-864

2003

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Synthetic Doppler tomograms of gas flows in the binary system IP Peg

Astronomy reports, 2001-11, Vol.45 (11), p.872-881

2001

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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

Astronomy reports, 2003-08, Vol.47 (8), p.621-636

2003

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Photometric parameters of the dwarf nova SS Cygni in the quiescent state

Astronomy reports, 2000-02, Vol.44 (2), p.89-102

2000

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Interpretation of light curves of IP Peg in a model with shockless interaction between the gas stream and disk

Astronomy reports, 2001-07, Vol.45 (7), p.538-552

2001

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Accretion disc in the massive V448 Cygni system

Monthly notices of the Royal Astronomical Society, 2009-07, Vol.396 (3), p.1553-1558

2009

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Accretion disc in the massive V448 Cygni system

Monthly notices of the Royal Astronomical Society, 2009, Vol.396 (3), p.1553-1558

2009

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Light-curve syntheses for close binary systems: Modeling spiral waves in an elliptical disk around a white dwarf

Astronomy reports, 2005, Vol.49 (10), p.783-800

KHRUZINA, T. S

2005

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Parameters of the X-ray binary system Scorpius X-1

Optical, J and K light curves of XTE J1118+480 = KV UMa: the mass of the black hole and the spectrum of the non-stellar component

I -band photometry of the quiescent black hole X-ray nova GROJ0422 + 32 = V518 Per: modelling of the orbital light curve and estimation of the black hole mass

Population synthesis of AX J1745.6−2901 X-ray nova-type binaries with rapidly decreasing orbital periods

Study of the Rapid Variability of a Dwarf Nova SS Cyg at Different Brightness Levels

Optical and J, K -photometry of the quiescent black hole X-ray nova A0620−00 in the passive and active states

Parameters of X-Ray Binary Sco X-1 in the Model of Partial Filling of Roche Lobe by Optical Star

Parameter Determination for the Eclipsing Long-Period Dwarf Nova EX Dra from Photometric Observations during Different Activity States of the System

Analysis of Photometric Observations of the New Cataclysmic Variable ASASSN-13cx

Photometric behavior of the cataclysmic variable SDSS J150240.98+333423.9/NZ Boo in quiescence

Light-curve syntheses for close binary systems: Modeling spiral waves in an elliptical disk around a white dwarf

Structure of the accretion disk in the cataclysmic variable UX uma in the transition to its quiescent state

The dwarf nova V1239 herculis in quiescence

Light-curve synthesis for close binaries: An extended shock as an analog of a hot spot in cataclysmic variables

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

Light-curve synthesis for close binaries: Elliptical disk around a white dwarf

Interpretation of light curves of the cataclysmic variable OY Car in a model with shockless interaction between a gaseous stream and the disk

Interpretation of orbital light curves of U Geminorum

Synthetic Doppler tomograms of gas flows in the binary system IP Peg

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

Photometric parameters of the dwarf nova SS Cygni in the quiescent state

Interpretation of light curves of IP Peg in a model with shockless interaction between the gas stream and disk

Accretion disc in the massive V448 Cygni system

Accretion disc in the massive V448 Cygni system

Light-curve syntheses for close binary systems: Modeling spiral waves in an elliptical disk around a white dwarf

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