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Просмотр Публикации сотрудников КФУ Scopus по автору "Fabrika S."

Просмотр Публикации сотрудников КФУ Scopus по автору "Fabrika S."

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  • Medvedev A.; Kholtygin A.; Hubrig S.; Schöller M.; Fabrika S.; Valyavin G.; Chountonov G.; Milanova Y.; Tsiopa O.; Yakovleva V. (2017)
    © 2017 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim We review the measurements of magnetic fields of OBA stars. Based on these data, we confirm that magnetic fields are distributed according to a lognormal law with mean ...
  • Fabrika S.; Ueda Y.; Vinokurov A.; Sholukhova O.; Shidatsu M. (2015)
    © 2015 Macmillan Publishers Limited. All rights reserved. The black hole mass and accretion rate in ultraluminous X-ray sources (ULXs) in external galaxies, whose X-ray luminosities exceed those of the brightest black holes ...
  • Kurtenkov A.; Pessev P.; Tomov T.; Barsukova E.; Fabrika S.; Vida K.; Hornoch K.; Ovcharov E.; Goranskij V.; Valeev A.; Molnár L.; Sárneczky K.; Kostov A.; Nedialkov P.; Valenti S.; Geier S.; Wiersema K.; Henze M.; Shafter A.; Muñoz Dimitrova R.; Popov V.; Stritzinger M. (2015)
    © ESO 2015. Context. M31N 2015-01a (or M31LRN 2015) is a red nova that erupted in January 2015 - the first event of this kind observed in M 31 since 1988. Very few similar events have been confirmed as of 2015. Most of ...
  • 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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