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  • Kostenkov A.; Vinokurov A.; Solovyeva Y.; Atapin K.; Fabrika S. (2020)
    © 2020, Pleiades Publishing, Ltd. Abstract: We calculate models of extended stellar atmospheres with a temperature in the range of 12 000–40 000 K and a mass loss rate of 10-6–10-4 Mʘyr-1. A large number of objects with ...
  • Solovyeva Y.; Vinokurov A.; Fabrika S.; Kostenkov A.; Sholukhova O.; Sarkisyan A.; Valeev A.; Atapin K.; Spiridonova O.; Moskvitin A.; Nikolaeva E. (2019)
    © 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. We have found three new luminous blue variable (LBV) candidates in the star-forming galaxy NGC4736. They show typical ...
  • Solovyeva Y.; Vinokurov A.; Sarkisyan A.; Atapin K.; Fabrika S.; Valeev A.F.; Kniazev A.; Sholukhova O.; Maslennikova O. (2020)
    © 2020 The Author(s). We search for luminous blue variable (LBV) stars in galaxies outside the Local Group. Here we present a study of two bright Hα sources in the NGC 247 galaxy. Object j004703.27-204708.4 (MV =-9.08 ± ...
  • Solovyeva Y.; Vinokurov A.; Sarkisyan A.; Kostenkov A.; Atapin K.; Fabrika S.; Oparin D.; Valeev A.; Bizyaev D.; Nedialkov P.; Spiridonova O. (2021)
    We continue to search for LBV stars in galaxies outside the Local Group. In this work, we have investigated four luminous stars in NGC 4449. Multiple spectral observations carried out for J122810.94+440540.6, J122811.70+440550.9, ...
  • Atapin K.; Fabrika S.; Caballero-García M. (2019)
    © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We analysed the X-ray power density spectra of five ultraluminous X-ray sources (ULXs) NGC5408 X-1, NGC6946 X-1, M82 ...
  • Atapin K.; Fabrika S.; Medvedev A.; Vinokurov A. (2015)
    © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. We study a stochastic variability of SS 433 in the 10-4-5 × 10-2 Hz frequency range based on RXTE data, and on simultaneous ...
  • Atapin K.; Fabrika S. (2016)
    © 2016, Pleiades Publishing, Inc.We study the X-ray variability of SS 433 based on data from the ASCA observatory and the MAXI and RXTE/ASM monitoring missions. Based on the ASCA data, we have constructed the power spectrum ...

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