Analysis of AAVSO Records of the Star Z Camelopardalis

Details Analysis of AAVSO Records of the Star Z Camelopardalis Analysis of AAVSO Records of the Star Z Camelopardalis

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006javso..35r.148o&link_type=abstract

The Journal of the American Association of Variable Star Observers, Vol. 35, No. 1, p. 148

Computer Science

Scientific paper

Z Camelopardalis is the prototype star of a subclass of dwarf nova that exhibit both outbursts and standstills. We use different statistical methods to gather as much data from the AAVSO record as possible about this star. Our data analysis focuses on three areas: correlations, long-term variations, and flux data. We compile the results from and compare these results to the most accepted model of Z Cam stars, the Meyer-Hoffmeister Theory.

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