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• W2149294906 abstract "We present spectroscopic and photometric observations of the cataclysmic variable CW 1045+525. Both the optical spectrum and the photometric lightcurve show a strong contribution of a K5V{M0V secondary. We derive an orbital period Porb =0 :271278(1) d by measuring the radial velocities of the absorption lines of the secondary. The period and spectral type of the secondary suggest a distance of 350{700 pc. There is evidence for additional sources of line- and continuum emission, but no direct evidence of an accretion disc. We discuss several scenarios for the nature of CW 1045+525 on the basis of our results, nding a dwarf nova classication to be the most probable, although not completely satisfying, explanation for the observed characteristics." @default.
• W2149294906 created "2016-06-24" @default.
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• W2149294906 date "2001-12-01" @default.
• W2149294906 modified "2023-10-14" @default.
• W2149294906 title "The cataclysmic variable CW 1045+525: A secondary-dominated dwarf nova?" @default.
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• W2149294906 doi "https://doi.org/10.1051/0004-6361:20011441" @default.
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