Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009a%26a...508l..17r&link_type=abstract
Astronomy and Astrophysics, Volume 508, Issue 1, 2009, pp.L17-L20
Astronomy and Astrophysics
Astrophysics
36
Stars: Abundances, Sun: Abundances, Planetary Systems
Scientific paper
We derive the abundance of 19 elements in a sample of 64 stars with fundamental parameters very similar to solar, which minimizes the impact of systematic errors in our spectroscopic 1D-LTE differential analysis, using high-resolution (R≃60 000), high signal-to-noise ratio (S/N≃200) spectra. The estimated errors in the elemental abundances relative to solar are as small as ≃0.025 dex. The abundance ratios [X/Fe] as a function of [Fe/H] agree closely with previously established patterns of Galactic thin-disk chemical evolution. Interestingly, the majority of our stars show a significant correlation between [X/Fe] and condensation temperature (T_C). In the sample of 22 stars with parameters closest to solar, we find that, on average, low TC elements are depleted with respect to high TC elements in the solar twins relative to the Sun by about 0.08 dex (≃20%). An increasing trend is observed for the abundances as a function of TC for 900
Asplund Martin
Melendez Jorge
Ramirez Ignacio
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