Abstract
The long-term CCD and photoelectric observations of YY Her covering the period of its post-outburst activity (JD 2 451 823 -2 452 996) are presented. We explain the periodic variations of the brightness of YY Her by the eclipses of the components in the system. The model with a deformed (non-homogeneous) envelope, surrounding the white dwarf is discussed. In addition, we observed a flare in about JD 2 452 440, during the primary minimum, that was later followed by an energetic outburst in JD 2 452 700.
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Hric, L., Gális, R., Niarchos, P., Gazeas, K. (2006). Symbiotic Binary YY Her — Eclipses, Flares and Outbursts. 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_76
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DOI: https://doi.org/10.1007/978-1-4020-5027-5_76
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