Physics
Scientific paper
Nov 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35389100l&link_type=abstract
VizieR On-line Data Catalog: J/A+A/538/A100. Originally published in: 2012A&A...538A.100L
Physics
Galaxies: Nearby, Stars: Giant, Abundances, Radial Velocities, Equivalent Widths, Photometry: Ubvri, Photometry: Infrared
Scientific paper
We use the VLT-FLAMES multi-fibre spectrograph in high-resolution mode (R~20000) to measure the abundances of several chemical elements, including Fe, Mg, Ca and Ba, in a sample of 35 individual Red Giant Branch stars in the Carina dwarf spheroidal galaxy. We also combine these abundances with photometry to derive age estimates for these stars. This allows us to determine which of two distinct star formation episodes the stars in our sample belong to, and thus to define the relationship between star formation and chemical enrichment during these two episodes.
(5 data files).
de Boer J. L. T.
Hill Vanessa
Irwin Mary Jane
Lemasle Bertrand
Salvadori Stefania
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