The SW Sextantis-type star 2MASS J01074282+4845188: an unusual bright accretion disk with non-steady emission and a hot white dwarf⋆

Author： Khruzina T.   Dimitrov D.   Kjurkchieva D.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|551|issue|A125-A125

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.551, Iss.issue, 2013-03, pp. : A125-A125

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Abstract

Context. Cataclysmic variables (CVs) present a short evolutional stage of binary systems. The nova-like stars are rare objects, especially those with eclipses (only several tens). But precisely these allow to determine the global parameters of their configurations and to learn more about the late stage of stellar evolution.

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