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Analysis of a selected sample of RR Lyrae stars in the LMC from OGLE-III TEXT SIZE: A A A
RR Lyrae stars are variables that pulsate in a well-understood way. The OGLE-III project is a continuation of a study that watches for changes in the brightness of stars over time. This article presents data of RR Lyrae observations associated with OGLE-III, contributing to knowledge in this field.
 
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