Abstract
New photoelectric and CCD observations of the eclipsing contact binary systems V344 Lac and V1191 Cyg are presented and analyzed. All available times of minimum light were used to study period changes of the systems and determine up-to-date ephemerides. The orbital period of V1191 Cyg is found to be increasing at a very fast rate. The photometric elements were determined using the new light curve, radial-velocity curve and broadening function fitting code ROCHE.
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Pribulla, T., Vaňko, M., Chochol, D., Parimucha, Š., Baluďanský, D. (2005). CCD Photometry of the Neglected Contact Binaries V344 Lac and V1191 Cyg. In: Drechsel, H., Zejda, M. (eds) Zdeněk Kopal’s Binary Star Legacy. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3875-5_41
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DOI: https://doi.org/10.1007/1-4020-3875-5_41
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Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-3131-1
Online ISBN: 978-1-4020-3875-4
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