The cyanogen distribution of the giants in 47 Tucanae

Details The cyanogen distribution of the giants in 47 Tucanae The cyanogen distribution of the giants in 47 Tucanae

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...230l.179n&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 230, June 15, 1979, p. L179-L182.

Astronomy and Astrophysics

Astrophysics

127

Abundance, Cyanogen, Globular Clusters, Red Giant Stars, Data Reduction, Data Sampling, Histograms, Nuclear Fusion

Scientific paper

Analysis of cyanogen measures of 142 stars on the red-giant branch of 47 Tucanae shows that the cyanogen distribution is preferentially bimodal, with the distribution becoming more cyanogen-rich toward the center. Most of the several observational constraints now available for 47 Tuc are suggestive of a primordial origin of its abundance anomalies, rather than of mixing.

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