Chaos in SS Cygni?

Details Chaos in SS Cygni? Chaos in SS Cygni?

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...334l..31c&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 334, Nov. 1, 1988, p. L31-L34. Research supported by McMaster Uni

Statistics

Computation

20

Chaos, Computational Astrophysics, Cygnus Constellation, Dwarf Novae, Light Curve, Strange Attractors, Cataclysmic Variables, Correlation, Statistical Analysis, Time Series Analysis

Scientific paper

A 21-yr stretch of the long-term American Association of Variable Star Observers (AAVSO) light curve of the dwarf nova SS Cygni is examined using standard techniques developed to search for an underlying chaotic attractor. The aim is to constrain the number of variables required to model the variations in the optical line flux. No evidence is found for a low-dimensional attractor.

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