Научные публикации в Scopus: Новые поступления

  • Zhuchkov R.; Malogolovets E.; Kiyaeva O.; Orlov V.; Bikmaev I.; Balega Y.; Safina D. (2010)
    An analysis of the physical characteristics, orbital parameters, and dynamical stability of the multiple Be star HD 217675 (o And) is presented. Observations on the 6-m SAO and 1.5-m RTT telescopes are used to refine the ...
  • Shimanskii V.; Karitskaya E.; Bochkarev N.; Galazutdinov G.; Lyuty V.; Shimanskaya N. (2012)
    Optical spectra and light curves of the massive X-ray binary V1357 Cyg are analyzed. The calculations were based on models of irradiated plane-parallel stellar atmospheres, taking into account reflection of the X-ray ...
  • Zhuchkov R.; Kiyaeva O.; Orlov V. (2010)
    Criteria for stability of triple systems are studied and compared with the results of numerical simulations obtained for model triple systems and observed multiple stars. The results for the stability analyses using two ...
  • Galeev A.; Bikmaev I.; Borisov N.; Zhuchkov R.; Shimanskii V.; Khabibullina M.; Sakhibullin N. (2008)
    We have carried out photometry and spectroscopy of the star V1327 Aql (R = 16 m ) as part of our program of observations of poorly studied cataclysmic variables using the 1.5-m optical Russian-Turkish telescope (RTT-150, ...
  • Zhuchkov R.; Malogolovets E.; Balega Y.; Bikmaev I.; Kuznetsov M.; Orlov V. (2008)
    We present the results of our study of the physical and dynamical parameters of the multiple system HD 222326. A new method for determining the individual radial velocities of components in wide binary and multiple systems ...
  • Shimanskii V.; Bikmaev I.; Borisov N.; Vlasyuk V.; Galeev A.; Sakhibullin N.; Spiridonova O. (2008)
    We present results of photometric and spectroscopic observations of four close binaries with subdwarf B components: PG 0918+029, PG 1000+408, PG 1116+301, PG 0001+275. We discovered that PG 1000+408 is a close binary, with ...
  • Shimanskii V.; Borisov N.; Pozdnyakova S.; Bikmaev I.; Vlasyuk V.; Sakhibullin N.; Spiridonova O. (2008)
    We have determined a complete set of parameters for the young pre-cataclysmic variable BE UMa from a comprehensive photometric and spectroscopic analysis using model atmospheres. Our precise photometry and spectroscopy ...
  • Morozova O.; Ratushnyak A.; Trushin M. (2012)
    Participation of planktonic and benthic bacteria in accumulation of polyphosphates in conditions of nitrates and phosphates overload was investigated in model mesocosms with natural water containing hydrobionts and curtains ...
  • Shimanskii V.; Borisov N.; Sakhibullin N.; Sheveleva D. (2008)
    We have classified and determined the parameters of the evolved close binary MT Ser. Our moderate-resolution spectra covering various phases of the orbital period were taken with the 6-m telescope of the Special Astrophysical ...
  • Abubekerov M.; Antokhina E.; Cherepashchuk A.; Shimanskii V. (2008)
    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 γ absorption line: m x = 1.8 M⊙ and mv = 2.5 M⊙. ...
  • Karitskaya E.; Bochkarev N.; Bondar A.; Galazutdinov G.; Lee B.; Musaev F.; Sapar A.; Shimanskii V. (2008)
    We discuss the results of optical spectroscopic monitoring of Cyg X-1 = HDE 226868/V1357 Cyg in 2002-2004. Our spectroscopy was carried out at the Terskol Observatory (Kabarda-Balkaria, Russia; the resolving power was R = ...
  • Suleimanov V.; Lipunova G.; Shakura N. (2007)
    Observations of X-ray binaries indicate substantial half-thicknesses for the accretion disks in these systems (up to h/R ≈ 0.25, where h is the disk half-thickness and R its radius), while standard α accretion disks predict ...
  • Kitiashvili I.; Gusev A. (2008)
    Assuming that the observed periodic variations of pulsar emission are due to the free precession of the spin axis, we investigate the evolution of the rotation of a two-layer neutron star using the Hamiltonian method of ...
  • Mashonkina L.; Vinogradova A.; Ptitsyn D.; Khokhlova V.; Chernetsova T. (2007)
    We derived Sr, Y, Zr, and Ce abundances for a sample of 74 cool dwarfs and subgiants with iron abundances, [Fe/H], between 0.25 and -2.43. These estimates were obtained using synthetic spectra, assuming local thermodynamic ...
  • Abubekerov M.; Antokhina E.; Cherepashchuk A.; Shimanskii V. (2006)
    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 optical star and screening of X-rays coming ...
  • Zhuchkov R.; Orlov V.; Rubinov A. (2006)
    We analyze the dynamical stability of the hierarchical quadruple systems HD 68255/6/7 and HD 76644 via numerical integration of the equations of motion of the four-body problem, with a chainlike regularization of close ...
  • Batalov R.; Valeev V.; Nuzhdin V.; Vorebev V.; Osin Y.; Lebedev D.; Bukharaev A.; Stepanov A. (2015)
    © 2015, Pleiades Publishing, Ltd. In this paper, a new technique is proposed for synthesis of porous silicon (PSi) layers with silver nanoparticles based on the method of low-energy high-dose metal ion implantation into ...
  • Bizyaev D.; Bukharaev A.; Ziganshina S.; Nurgazizov N.; Khanipov T.; Chuklanov A. (2015)
    © 2015, Pleiades Publishing, Ltd. The experimental results on scanning probe lithography (SPL)—the formation of lithographic masks using scanning probe microscope—are presented. Polymethylmethacrylate (PMMA)-based masks ...
  • Tkachenko L. (2014)
    Nonlinear gas oscillations excited in a tube with an open end by a piston driven by a crank mechanism are investigated. For the open end of the tube, a nonlinear boundary condition is formulated with allowance for oscillations ...
  • Safiullin L.; Bagautdinova N.; Safiullin N.; Ismagilova G. (2012)
    In work on the basis of revealing of interconnection between theories of welfare and markets of imperfect competition, by quality non-homogeneity of goods and services, consumers and producers there determines the influence ...

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