Iron abundances of red giants in Carina gal. Virtual Observatory Resource

Authors

1. Fabrizio M.
2. Merle T.
3. Thevenin F.
4. Nonino M.
5. Bono G.
6. Stetson P.B.,Ferraro I.
7. Iannicola G.
8. Monelli M.
9. Walker A.R.
10. Buonanno R.
11. Caputo F.,Corsi E.
12. Dall'Ora M.
13. Degl'Innocenti S.
14. Francois P.
15. Gilmozzi R.,Marconi M.
16. Pitrinferni A.
17. Prada Moroni P.G.
18. Primas F.
19. Pulone L.,Ripepi V.
20. Romaniello M.

Published by

CDS

Abstract

We have performed accurate iron abundance measurements for 44 red giants (RGs) in the Carina dwarf spheroidal (dSph) galaxy. We used archival, high-resolution spectra (R~38000) collected with UVES at ESO/VLT either in slit mode (five RGs) or in fiber mode (39 RGs, FLAMES/GIRAFFE-UVES). The sample is more than a factor of 4 larger than any previous spectroscopic investigation of stars in dSphs based on high-resolution (R>=38000) spectra.

Keywords

1. giant-stars
2. chemical-abundances

Bibliographic source Bibcode

2012PASP..124..519F

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