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Paper: Pulsation of the AGB Variable in the Symbiotic Nova PU Vulpeculae
Volume: 203, The Impact of Large-Scale Surveys on Pulsating Star Research, IAU Colloquium 176
Page: 125
Authors: Chochol, D.; Pribulla, T.
Abstract: Analysis of the 1993-4 eclipse in the slow symbiotic nova PU Vul (4900-d binary orbital period) and 1995-9 photoelectric observations in V and R bandpasses show that the cool component of this object is pulsating AGB variable with a 215-d pulsation period. Basic properties of the components of the system are discussed.
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