Metal abundance of the intermediate-age open cluster NGC 3532

Details Metal abundance of the intermediate-age open cluster NGC 3532 Metal abundance of the intermediate-age open cluster NGC 3532

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988obs...108..218c&link_type=abstract

The Observatory, vol. 108, p. 218-220 (1988)

Physics

5

Scientific paper

Washington photometry for a sample of red giants in the open cluster NGC 3532 is presented. The Fe+CNO-sensitive Δ(M-T1) and CN-contaminated Δ(C-M) abundance indices yield results in excellent agreement ([Fe/H] ≅ 0.1). No CN strength variations are detected among the cluster giants. The authors conclude that NGC 3532, with a nearly solar metal content, lies on the metal-rich side of the distribution of intermediate-age open clusters.

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