Abstract
An investigation of the observational properties for RR Lyrae variables in the galactic globular cluster ω Centauri is reported. The results show that ω Centauri belongs to the Oosterhoff Group I, notwithstanding the large, Oo II-like value of the average of the periods of ab-type RR Lyrae. The helium content is derived for this cluster from the analysis of the variables in the (A-logT e) plane. It is shown that the helium abundance is very close to the value Y=0.30, about 0.05 larger than the value derived for the ‘normal’ Oo I globular cluster M3.
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Caputo, F. The helium content of the peculiar Oosterhoff type I globular cluster ω Centauri. Astrophys Space Sci 76, 329–339 (1981). https://doi.org/10.1007/BF00687497
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DOI: https://doi.org/10.1007/BF00687497