@inproceedings{326345b30fa742cfbb79bede2657238f,
title = "The Nature of the Metal-Rich Thick Disk",
abstract = "We have traced the Galactic thick disk to its, to date, highest metallicities. Based on high-resolution spectroscopic observations of 187 F and G dwarf stars that kinematically can be associated either with the thin disk (60 stars) or with the thick disk (127 stars), we find that the thick disk stars reach at least solar metallicities, and maybe even higher. This finding is independent of the U\_LSR, V\_LSR and W\_LSR velocities of the stars.",
author = "T. Bensby and A.R. Zenn and M.S. Oey and Sofia Feltzing",
year = "2007",
language = "English",
isbn = "978-1-58381-309-6",
volume = "374",
publisher = "Astronomical Society of the Pacific (ASP)",
pages = "181--186",
editor = "Antonella Vallenari and et al.",
booktitle = "ASP Conference Proceedings",
address = "United States",
note = "From stars to galaxies: Building the pieces to build up the universe ; Conference date: 16-10-2006 Through 20-10-2006",
}