Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396...63f&link_type=abstract
Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at
Astronomy and Astrophysics
Astronomy
Scientific paper
Clues to the early formation of the Milky Way disk are preserved within the detailed stellar abundances of its most metal-poor stars. Only a few metal-poor disk stars with [Fe/H] < -1 have been analyzed for their abundances until now. We have observed a large sample (> 75 stars) of metal-poor disk stars isolated from the catalog of the RAdial Velocity Experiment (RAVE). While the analysis is ongoing, we have confirmed that a significant metal-poor disk population with an alpha-element enhancement slightly greater than the local stellar halo. This suggests an early and rapid formation for these stars.
Fulbright Jon P.
Ruchti Gregory
~Wyse Rosemary F. G.
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