Просмотр по теме "Novae"

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  • Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disks 
    Revnivtsev M.; Burenin R.; Bikmaev I.; Kniazev A.; Buckley D.; Pretorius M.; Khamitov I.; Ak T.; Eker Z.; Melnikov S.; Crawford S.; Pavlinsky M. (2010)
    We study the power spectra of the variability of seven intermediate polars containing magnetized asynchronous accreting white dwarfs, XSS J00564+4548, IGR J00234+6141, DO Dra, V1223 Sgr, IGR J15094-6649, IGR J16500-3307 ...
  • Dwarf nova EZ Lyncis second visit to instability strip 
    Pavlenko E.; Kato T.; Sosnovskij A.; Andreev M.; Ohshima T.; Sklyanov A.; Bikmaev I.; Galeev A. (2013)
    © 2014 © The Author 2014. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved. The analysis of 14 periodograms of EZLyn for data spaced over 565d in 2012-2014 (2-3.5yr ...
  • Statistics of white dwarf properties in intermediate polars 
    Suleimanov V.F.; Doroshenko V.A.; Werner K. (2020)
    © The Author(s), 2020. Many intermediate polars are hard X-ray sources. The theory of their hard X-ray radiation is well developed and allows us to determine white dwarf masse in this kind of cataclysmic variables. Here ...
  • The January 2015 outburst of a red nova in M 31 
    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 ...

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