Abstract
ABSTRACT An analysis of the CNO and s-process abundances in the M22 star III-106 has been completed. This star has been identified on the basis of DDO photometry by Hesser, Hartwick, and McClure, and on the basis of a low-resolution spectrum by McClure and Norris as a CH star. We find the star to have C = 7.1, N = 7.65,.
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