Other
Scientific paper
Feb 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87..360s&link_type=abstract
Astronomical Journal, vol. 87, Feb. 1982, p. 360-368.
Other
26
Giant Stars, Heavy Elements, Interstellar Extinction, Open Clusters, Stellar Evolution, Stellar Spectra, Stellar Spectrophotometry, Abundance, Cyanogen, Metallic Stars, Spectrum Analysis, Star Distribution, Ubv Spectra
Scientific paper
DDO photometry has been obtained for 14 stars in the open cluster IC 4651. The reddening and distance modulus derived from these data are in good agreement with the results obtained from UBV photometry by Eggen. The cluster appears to have a heavy-element abundance slightly less than that of the Hyades, although one giant shows an anomalously strong 4216-A CN band comparable to those seen in the SMR giants. A comparison is made between this star and CN-enhanced giants in eight other open clusters. It is suggested that the CN-strong phenomenon among open cluster giants is the result of nonstandard stellar evolution, the occurrence of which is supported by the presence of blue stragglers in five out of the eight comparison clusters, as well as in IC 4651 itself.
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