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- W1972534982 abstract "To compare the globular clusters (GCs) associated with the Sagittarius Galaxy (Sgr) we report the results obtained from new high-resolution spectra of red giant stars in Terzan 8 and Arp 2, collected with the Magellan Inamori Kyocera Echelle (MIKE) spectrograph at Las Campanas Observatory. For Ter 8 we find [Fe i/H] = −2.37 ± 0.04 and [Fe ii/H] = −2.30 ± 0.07, while for Arp 2 [Fe i/H] = −1.77 ± 0.04 and [Fe ii/H] = −1.89 ± 0.07. Other elements, usually of interest, show the following results. For oxygen, we obtain [O/Fe] = 0.71 ± 0.17 for Ter 8 and [O/Fe] = 0.21 ± 0.22 for Arp 2. For the α-elements (Mg, Si, Ca, Ti), the mean values are 037 ± 0.14 dex for Ter 8 and 0.31 ± 0.11 for Arp 2. These values are not too different from the Galactic GCs at a similar [Fe/H] value. Regarding Cu, we find quite underabundant results for both clusters: [Cu/Fe] = −0.96 for Ter 8 and [Cu/Fe] = −0.93 for Arp 2. The heavy s-process elements Ba and Nd show no excesses in Ter 8 and Arp 2. Our only r-process element, Eu, shows an excess of 0.45 dex in Arp 2, based on the only useful line at 6645 Å." @default.
- W1972534982 created "2016-06-24" @default.
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- W1972534982 date "2008-07-02" @default.
- W1972534982 modified "2023-09-26" @default.
- W1972534982 title "ARP 2 AND TERZAN 8: A DETAILED CHEMICAL ANALYSIS" @default.
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- W1972534982 doi "https://doi.org/10.1088/0004-6256/136/2/614" @default.
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