Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 356, Issue 4, Pages 1276-1282Publisher
BLACKWELL PUBLISHING LTD
DOI: 10.1111/j.1365-2966.2004.08529.x
Keywords
techniques : spectroscopic; stars : abundances; stars : late-type; Galaxy : bulge; globular clusters : individual : NGC 6342; globular clusters : individual : NGC 6528
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Using the Near Infrared Spectrometer (NIRSPEC) spectrograph at Keck II, we have obtained infrared (IR) echelle spectra covering the range 1.5-1.8 mum for the moderately reddened bulge globular clusters NGC6342 and 6528, finding [Fe/H] = -0.60 and -0.17 dex, respectively. We measure an average alpha-enhancement of approximate to+0.33 dex in both clusters, consistent with previous measurements on other metal-rich bulge clusters, and favouring the scenario of a rapid bulge formation and chemical enrichment. We also measure very low C-12/C-13 isotopic ratios (approximate to5 in NGC 6342 and approximate to8 in NGC 6528), suggesting that extra-mixing mechanisms resulting from cool bottom processing are at work during evolution along the red giant branch (RGB).
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