A 116 Year Record of Mass Transfer in R Arae

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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5 pages, 3 figures, accepted for publication in IBVS on Feb. 14, 2011

Scientific paper

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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