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Cycle-to-cycle changes in the Mira-type star RT Cyg
Published online by Cambridge University Press: 25 May 2016
Abstract
The moments of 82 maxima and 76 minima are used for the correlation analysis of the characteristics of the individual cycles. 5 not trivial correlations were found. The characteristic time of the secular decrease of the period is |P/P| = (23.4 ± 4.3) · 103 yrs, but decade–scale and cycle–to–cycle variations are also present.
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- V. From AGB to Planetary Nebulae
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- Copyright © Kluwer 1997