Analysis of the Light Curve of the RV Tauri Star LV Del

Physics

Scientific paper

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Scientific paper

We present the V magnitude light curve of the RV Tauri Star LV Del. Analysis reveals longterm variation in brightness, identifying it as a member of the RVb subclass. The star appears to be experiencing a phase where the formal RV Tauri character is poorly expressed, and the behavior is more ``Cepheid-like.'' Non-linear time series analysis reveals the presence of low dimensional chaos.

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