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  1. Article

    Open Access

    Distribution of Cool Starspots on the Surface of the Red Dwarf V647 Her

    An analysis of photometric observations of the star V647 Her (M3.5V) obtained at the 1.25-m telescope of the Crimean Astrophysical Observatory in 2022 is presented. The presence of a low-amplitude variability ...

    N. I. Bondar’, K. A. Antonyuk, N. V. Pit, I. Yu. Alekseev in Astronomy Reports (2024)

  2. Article

    Open Access

    Characteristics of Long-Term Spot Activity on Several Late-Spectral-Type Stars

    We present our analysis of many-year photometry for several dozens of chromospherically active stars that exhibit solar-type activity (from our own observations as well as from data in the literature). Modelin...

    A. V. Kozhevnikova, I. Yu. Alekseev, V. P. Kozhevnikov in Astronomy Reports (2023)

  3. No Access

    Article

    Circumstellar Properties of the Herbig Be Star HD 259431. I. Signatures of Magnetospheric Accretion

    Results are presented from a spectroscopic study of the Ae/Be Herbig star HD 259431 conducted from 2010 to 2019 using high-resolution spectrographs at: (a) the Crimean Astrophysical Observatory, (b) European S...

    M. A. Pogodin, S. E. Pavlovskii, N. G. Beskrovnaya, N. A. Drake in Astrophysics (2022)

  4. No Access

    Article

    Analysis of the Spectroscopic Observations of RS CVn Type Star V837 Tau

    We present an analysis of the spectra of the star V837 Tau, which belongs to a class of chromosphere-active RSCVn type stars. The observational material was obtained with the 1.5-m Russian-Turkish telescope RT...

    A. I. Kolbin, V. V. Shimansky, I. Yu. Alekseev, N. N. Shimanskaya in Astrophysical Bulletin (2019)

  5. No Access

    Article

    Features of the Wind of the Unique Herbig Ae Star HD 190073

    Results of our spectral monitoring of the Herbig Ae star HD190073 during 2009-2017 at the Crimean Astrophysical Observatory are presented. Over this time, 116 spectra were obtained in the region of the Hα line...

    O. V. Kozlova, M. A. Pogodin, I. Yu. Alekseev, M. I. Dombrovskaya in Astrophysics (2019)

  6. No Access

    Article

    Short-Term Spectral Variability of the Herbig Ae/Be Star HD37806

    The spectroscopic variability of the Herbig Ae/Be star HD 37806 is analyzed on temporal scales from night-to-night, and over individual nights. The observations were made during November 2012 on the ASP-14 Cou...

    M. A. Pogodin, O. V. Kozlova, I. Yu. Alekseev, S. E. Pavlovskiy in Astrophysics (2019)

  7. No Access

    Article

    Long-term Spot-Coverage Variations of 13 BY Dra G–K Dwarfs

    The results of spot-coverage modeling for 13 active G–K dwarf stars based on many-year photometric observations are presented. The results of UBVRI observations of eight stars performed at the Crimean Astrophysic...

    I. Yu. Alekseev, A. V. Kozhevnikova in Astronomy Reports (2018)

  8. No Access

    Article

    Photospheric Spots and Flare on the Active Dwarf Star FR Cnc

    We perform analysis of new BVRI photometry of young active dwarf star FR Cnc (K7V), obtained at Kourovka astronomical observatory of Ural Federal University with the help of multichannel electrophotometer in F...

    A. V. Kozhevnikova, V. P. Kozhevnikov, I. Yu. Alekseev in Astrophysics (2018)

  9. No Access

    Article

    Spectral Variability of the Herbig Ae/Be Star HD 37806

    Results are reported from a spectroscopic study of the Herbig Ae/Be star HD 37806 from 2009 through 2017 using high resolution spectrographs at the Crimean Astrophysical Observatory and the OAN SPM Observatory...

    M. A. Pogodin, S. E. Pavlovskiy, O. V. Kozlova, N. G. Beskrovnaya in Astrophysics (2018)

  10. No Access

    Article

    Long-Term Spectral Variability of the Spotted Star in Com

    High-resolution (R = 20000) spectral observations over many years of the spotted star IN Com in the regions of the Hα, Hβ, and He I 5876 Å lines are reported. The distinctive feature of the spectrum of this st...

    O. V. Kozlova, I. Yu. Alekseev, A. V. Kozhevnikova in Astrophysics (2017)

  11. No Access

    Article

    Long-term variations in the spottedness of BY Dra M dwarfs

    The results of a spottedness study for twelve red dwarf stars covering several decades and based on a vast amount of photometric observations are presented. The analysis makes use of multicolor (UBV RI) photometr...

    I. Yu. Alekseev, A. V. Kozhevnikova in Astronomy Reports (2017)

  12. No Access

    Article

    Long-term spottedness variations of 16 RS CVn stars

    An improved zonal model for spotted stellar photospheres enabling analysis of two active longitudes simultaneously present on a star is used to determine the spottedness parameters for a sample of chromospheri...

    A. V. Kozhevnikova, I. Yu. Alekseev in Astronomy Reports (2015)

  13. No Access

    Article

    Three-Component Model of Spottedness in the Classical RS CVn System UX Ari

    It is shown that the hypothesis of a complex (cold spots and hot flares) structure for the active regions on UX Ari reproduces well the photometric behavior of the star. According to the model the spots are co...

    I. Yu. Alekseev in Astrophysics (2014)

  14. No Access

    Article

    Starspots and active regions on IN Com: UBVRI photometry and linear polarization

    The activity of the variable star IN Com is considered using the latest multicolor UBVRI photometry and linear polarimetric observations carried out during a decade. The photometric variability of the star is ...

    I. Yu. Alekseev, O. V. Kozlova in Bulletin of the Crimean Astrophysical Observatory (2014)

  15. No Access

    Article

    The stellar wind as a key to the understanding of the spectral activity of IN Com

    We present long-term spectral observations (R = 20000) of IN Com in the region of the Hα, Hβ, and He I 5876 lines. One distinguishing characteristic of the stellar spectrum is the presence in the Hα line of an ex...

    O. V. Kozlova, I. Yu. Alekseev in Bulletin of the Crimean Astrophysical Observatory (2014)

  16. No Access

    Article

    Starspots on Young pms Stars

    Long-term, multiband photometric observations of 8 young PMS stars are used to construct models for their starspots. It is shown that the average density of starspots is up to 40 % of the total surface of a st...

    I. Yu. Alekseev in Astrophysics (2014)

  17. No Access

    Article

    Role of molybdenum in increasing the resistance of steel to the breaking effect of hydrogen at elevated temperatures and pressures (hydrogen corrosion)

    The physicochemical nature and the mechanism of the breaking effect of hydrogen on steel at elevated temperatures and pressures (hydrogen corrosion) are studied. This phenomenon is found to be based on the che...

    V. I. Alekseev, V. S. Yusupov, G. Yu. Lazarenko in Russian Metallurgy (Metally) (2013)

  18. No Access

    Article

    Spot activity of the binary CG Cyg: Observations during maximum spottedness

    We present the results of new multicolor photometry of the chromospherically active binary CG Cyg acquired in 2005–2009 (136 hours of observations). The light curves for each season reveal rotational brightnes...

    A. V. Kozhevnikova, V. P. Kozhevnikov, I. Yu. Alekseev, I. A. Yushkov in Astronomy Reports (2012)

  19. No Access

    Article

    Topokinetic model of active dissolution of a solid electrode with point lattice defects. analysis and comparison of the results obtained in solving equations with the experimental data

    A model that takes into account the consistence between the atomic relief with the metal dissolution (corrosion) rate and also considers the direct effect of point lattice defects (vacancies or atoms of impuri...

    Yu. V. Alekseev, A. V. Plaskeev, I. Yu. Alekseev in Russian Journal of Electrochemistry (2012)

  20. No Access

    Article

    Long-term starspot activity of the eclipsing binaries BH Vir and WY Cnc

    We present the results of multicolor photometry of the two spotted, short-period, late-type RS CVn stars BH Vir and WY Cnc. We have derived the parameters of the binaries’ components, and refined their masses,...

    A. V. Kozhevnikova, I. Yu. Alekseev, P. A. Heckert, V. P. Kozhevnikov in Astronomy Reports (2007)

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