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- W2034659610 abstract "Eddington during the years of pioneering in General Relativity worked also in observational statistics of variable stars, and proposed a model for Cepheids' pulsation. The statistical analysis of time series of long-period variable stars (Mira): Mira Ceti and x Cygni made by Eddington and Plakidis in 1929 has been extended to luminosities dominion and to R Leonis and R Hydrae, The difference between consecutive maxima AM is negatively correlated with the magnitude M of the first maximum of the pair. Bright maxima are preferentially followed by dim ones, excepted for R Hydrae. It shows a possible two-periods time pattern of its maxima, which makes easier predictions of its maxima. Our two-points correlation analysis is still not enough to give a satisfactory predictive model of maxima sequence." @default.
- W2034659610 created "2016-06-24" @default.
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- W2034659610 date "2006-02-01" @default.
- W2034659610 modified "2023-09-23" @default.
- W2034659610 title "CORRELATION OF MAXIMA IN LONG-PERIOD VARIABLE STARS: FROM EDDINGTON TO PRESENT TIME" @default.
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- W2034659610 doi "https://doi.org/10.1142/9789812704030_0266" @default.
- W2034659610 hasPublicationYear "2006" @default.
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