Deep Mixing Statistics in the Globular Cluster NGC5466

Details Deep Mixing Statistics in the Globular Cluster NGC5466 Deep Mixing Statistics in the Globular Cluster NGC5466

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21547813w&link_type=abstract

American Astronomical Society, AAS Meeting #215, #478.13; Bulletin of the American Astronomical Society, Vol. 42, p.567

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Scientific paper

Using VIRUS-P in conjunction with the 2.7m telescope at McDonald Observatory, we obtained a sample of red giants from the metal-poor globular cluster NGC 5466. The flux of the CN and CH absorption features was calculated using the band indices S3839 and SCH respectively. The results indicate that none of the red giants in this sample exhibit deep mixing abundances. To date all similarly surveyed globular clusters show at least some stars with deep mixing abundances. We discuss the cluster properties of NGC 5466 and how this lack of deep mixing stars makes NGC 5466 different from other metal-poor globular clusters.

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