2015
DOI: 10.1088/0004-6256/149/3/90
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UBVRIANALYSIS OF THE TOTALLY ECLIPSING EXTREME MASS RATIO W UMa BINARY, GSC 3208 1986

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Cited by 5 publications
(8 citation statements)
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“…The temperature of the more massive component was found to be about 200 K cooler than the less massive one. The main parameters obtained in this study were similar to the results of Samec et al (2009). But our fit applied a cool spot on the more massive component, corresponding to the characteristic of the asymmetric light curves.…”
Section: Photometric Solutionssupporting
confidence: 81%
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“…The temperature of the more massive component was found to be about 200 K cooler than the less massive one. The main parameters obtained in this study were similar to the results of Samec et al (2009). But our fit applied a cool spot on the more massive component, corresponding to the characteristic of the asymmetric light curves.…”
Section: Photometric Solutionssupporting
confidence: 81%
“…New observations in BVR filter bands showed asymmetric light curves to be a negative type of the O'Connell effect, which can be described by magnetic activity of a cool spot on the more massive component. Our photometric solutions showed that V873 Per is a W-type with a mass ratio of q = 2.504(±0.0029), confirming the results of Samec et al (2009). The derived contact degree was found to be f = 18.10%(±1.36%).…”
supporting
confidence: 81%
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