Fadings of R Coronae Borealis stars - Random or chaotic?

Details Fadings of R Coronae Borealis stars - Random or chaotic? Fadings of R Coronae Borealis stars - Random or chaotic?

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...252..701d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 252, no. 2, Dec. 1991, p. 701-704.

Astronomy and Astrophysics

Astrophysics

6

Chaos, Corona Borealis Constellation, Late Stars, Stellar Luminosity, Stellar Spectrophotometry, Variable Stars, Absorption Spectra, Pulsars, Stellar Color, Stellar Mass

Scientific paper

The timings of the fades of four R Coronae Borealis stars are analyzed
for characteristics of systems driven by a low-dimensional attractor. R
CrB, RY Sgr, and S Aps have interfade timings which have a high
probability of being truly random. However, the analysis of SU Tau
implies that a determinable mechanism is responsible for the fades.

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