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Elemental abundances in the Galactic bulge from microlensed dwarf stars

Bensby, T. and Feltzing, S. and Johnson, J.~A. and Gould, A. and Sana, H. and Gal-Yam, A. and Asplund, M. and Lucatello, S. and Melendez, J. and Udals

Keywords

Astrophysics - Galaxy Astrophysics

Abstract

We present elemental abundances of 13 microlensed dwarf and subgiant stars in the Galactic bulge, which constitute the largest sample to date. We show that these stars span the full range of metallicity from Fe/H=-0.8 to _s160.4, and that they follow well-defined abundance trends, coincident with those of the Galactic thick disc.

Information

Published
2009 as article
ArXiv e-prints, to be published on A_s13A,
Type
experimental work
Links
pdf
adsabs.harvard.edu/a…
Related to the research area(s):
G
e-Print
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Exzellenzcluster Universe

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