Abstract
We have re-analyzed old photometric UBV data obtained by Papoušek et al. at Skalnaté Pleso, Slovakia (1967–1980) and Brno, Czech Republic (1976–1979) observatories and analyzed new own CCD measurements (Brno, 2003–2005). In both set of photometric data the oscillations in the vicinity of the primary minimum were found. The detected periods are compatible with the previously published ones.
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Zejda, M., Mikulàšek, Z., Wolf, M., Pejcha, O. (2006). Short Time-Scale Variability in the Light Curve of TW Draconis. In: Giménez, À., Guinan, E., Niarchos, P., Rucinski, S. (eds) Close Binaries in the 21st Century: New Opportunities and Challenges. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5027-5_39
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DOI: https://doi.org/10.1007/978-1-4020-5027-5_39
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