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• W2129864066 abstract "We have analyzed high-resolution echelle spectra of red giant members for seven open clusters in the Galactic anticentre direction to explore their chemical positions. Cluster membership has been confirmed by radial velocity. The spread in temperatures and gravities being very small among the red giants, nearly the same stellar lines were employed for all stars thereby reducing the abundance errors: the errors of the average abundance for a cluster were generally in the 0.02 to 0.05 dex range. Our present sample covers Galactocentric distances of 8.3 to 11.3 kpc and an age range of 0.2 to 4.3 Gyr. A careful comparison of our results for the cluster NGC 2682 (M 67) to other high-resolution abundance studies in the literature shows general good agreement for almost all elements in common." @default.
• W2129864066 created "2016-06-24" @default.
• W2129864066 creator A5020600710 @default.
• W2129864066 creator A5034985884 @default.
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• W2129864066 date "2013-04-11" @default.
• W2129864066 modified "2023-09-24" @default.
• W2129864066 title "Comprehensive abundance analysis of red giants in the open clusters NGC 2527, 2682, 2482, 2539, 2335, 2251 and 2266" @default.
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• W2129864066 doi "https://doi.org/10.1093/mnras/stt412" @default.
• W2129864066 hasPublicationYear "2013" @default.
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