- Elemental abundances in the Galactic bulge from microlensed dwarf stars
- IAU Symposium
- Pages (from-to)
- Document type
- Faculty of Science (FNWI)
- Anton Pannekoek Institute for Astronomy (API)
- 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 +0.4, and that they follow well-defined abundance trends, coincident with those of the Galactic thick disc.
- go to publisher's site
- ID: 642
Proceedings title: Chemical abundances in the universe: connecting first stars to planets: Proceedings of the 265th Symposium of the International Astronomical Union held in Rio de Janeiro, Brazil, August 10-14, 2009
Publisher: Cambridge University Press
Place of publication: Cambridge
Editors: K. Cunha, M. Spite, B. Barbuy
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