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A 116 Year Record of Mass Transfer in R Arae
classification
🌌 astro-ph.SR
keywords
araedataephemerismasstransferanalysisarchivalaverage
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This is a period study of the bright interacting southern eclipsing binary star R Arae. New photometric data are combined with archival data to determine R Ara's average mass transfer rate over the past 116 years through the analysis of the resulting ephemeris curve. An updated ephemeris is given.
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