Physics
Scientific paper
Nov 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ibvs.5804....1m&link_type=abstract
Information Bulletin on Variable Stars, 5804, 1.
Physics
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.
Honeycutt Kent R.
Maderak Ryan M.
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