SS Cygni Outburst Predictors and Long Term Quasi-periodic Behavior

Details SS Cygni Outburst Predictors and Long Term Quasi-periodic Behavior SS Cygni Outburst Predictors and Long Term Quasi-periodic Behavior

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007pasp..119.1361p&link_type=abstract

Publications of the Astronomical Society of the Pacific, Volume 119, issue 862, pp.1361-1366

Astronomy and Astrophysics

Astronomy

Stars

Scientific paper

We report null results on a 2 year photometric search for outburst predictors in SS Cyg. Observations in Johnson V and Cousins I were obtained almost daily for multiple hours per night for two observing seasons. The accumulated data are put through various statistical and visual analysis techniques, but we fail to detect any outburst predictors. However, analysis of 102 years of AAVSO archival visual data has led to the detection of a correlation between a long term quasi-periodic feature at around 1000-2000 days in length and an increase in outburst rate.

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