The nature of the metal-rich thick disk

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dc.creatorBensby, T.
dc.creatorZenn, A. R.
dc.creatorOey, M. S.
dc.creatorFeltzing, S.
dc.date2006-12-16
dc.date.accessioned2026-07-07T07:35:49Z
dc.date.available2026-07-07T07:35:49Z
dc.descriptionWe 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.
dc.description6 pages, to appear in proceedings for "From stars to galaxies: Building the pieces to build up the Universe" conference, held in Venice, 16-20 October 2006, A. Vallenari, R. Tantali, L. Portinari, A. Moretti (eds), ASP Conf Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/0612459
dc.identifierhttp://arxiv.org/abs/astro-ph/0612459
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120220
dc.subjectAstrophysics
dc.titleThe nature of the metal-rich thick disk
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