most citedMultiple time scales in cataclysmic binaries. The low-field magnetic dwarf nova DO Draconis

16 citations · 39 across the 4 of their papers we have counts for

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astro-ph200817 cited

Nova-Like Cataclysmic Variable TT Ari: QPO Behaviour Coming Back From Positive Superhumps

Y. Kim, I. L. Andronov, S. M. Cha +1

We study the variability of the nova-like cataclysmic variable TT Ari, on time-scales of between minutes and months. The observations in the filter R were obtained at the 40-cm tel…

astro-ph200816 cited

Multiple time scales in cataclysmic binaries. The low-field magnetic dwarf nova DO Draconis

I. L. Andronov, L. L. Chinarova, W. Han +2

We study the variability of the cataclysmic variable DO Dra, on time-scales of between minutes and decades. The characteristic decay time dt/dm=0.902(3) days/mag was estimated from…

astro-ph20087 cited

Idling Magnetic White Dwarf in the Synchronizing Polar BY Cam. The Noah-2 Project

Ivan L. Andronov, Kirill A. Antoniuk, Vitalii V. Breus +8

Results of a multi-color study of the variability of the magnetic cataclysmic variable BY Cam are presented. The observations were obtained at the Korean 1.8m and Ukrainian 2.6m, 1…

astro-ph2005

Orbital and spin variability of the Intermediate Polar BG CMi

Y. G. Kim, I. L. Andronov, S. S. Park +1

Results of a CCD study of the variability of the cataclysmic variable BG CMi obtained at the Korean 1.8m telescope in 2002-2005 are presented. The "multi-comparison star" method ha…

astro-ph2004

Discovery of a bright X-ray transient in the Galactic Center with XMM-Newton

D. Porquet, N. Grosso, V. Burwitz +4

We report the discovery of a bright X-ray transient object, XMMU J174554.4-285456, observed in outburst with XMM-Newton on October 3, 2002,and located at 6.3' from SgrA*, the super…

astro-ph2003

Blobby accretion in magnetic cataclysmic variables

A. V. Halevin, I. L. Andronov, N. M. Shakhovskoy +2

The processes of accretion of the gaseous blobs with different masses and densities onto strongly magnetized white dwarfs in the systems of polars have been modeled. We have proved…