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Home All issues Volume 538 (February 2012) A&A, 538 (2012) A100 Full HTML
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Fig. 10

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The ages (in Gyr) as a function of [Fe/H] (dex) for the RGB stars with high resolution abundances in the Carina dSph (see also Table 10). The shaded areas represent the expected age ranges of star formation as indicated by photometric studies.

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