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- W320895983 abstract "When the reciprocal periods change linearly with time, three widely separated epochs are sufficient to calculate the rate of change and the present period. This method is tested on variables of the globular clusters Cen, M 3, and M 5. In addition, new epochs are given for three W UMa eclipsing binaries and two RR Lyr variables not belonging to clusters. The periods of the latter are found to be changing somewhat faster than those of the globular-cluster variables. Key words: period changes - photometry - W UMa stars - RR Lyrae stars" @default.
- W320895983 created "2016-06-24" @default.
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- W320895983 date "1976-08-01" @default.
- W320895983 modified "2023-10-11" @default.
- W320895983 title "Redetermination of periods of variable stars UZ Leo,V502 Oph, WZ Hya,UY Boo, and YY Eri." @default.
- W320895983 doi "https://doi.org/10.1086/129980" @default.
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