Our samples are composed by Milky Way field stars and stars in open clusters. The former sample includes stars observed with the UVES set-up centred around 580.0nm, which belong to the solar neighbourhood and inner disc samples. We divided the field stars into thin and thick disc stars, using their [alpha/Fe] abundance ratio, following the approach of Adibekyan et al. (2011A&A...535L..11A). Our sample includes 19 thin disc stars and 130 thick disc stars with both N and O measurements. Their stellar parameters and the abundances of N and O are listed in tablea1.dat. (2 data files). ...
VizieR Online Data Catalog: GES N/O abundance ratio in the Milky Way (Magrini+, 2018)
Lanzafame, A. C.;
2018-01-01
Abstract
Our samples are composed by Milky Way field stars and stars in open clusters. The former sample includes stars observed with the UVES set-up centred around 580.0nm, which belong to the solar neighbourhood and inner disc samples. We divided the field stars into thin and thick disc stars, using their [alpha/Fe] abundance ratio, following the approach of Adibekyan et al. (2011A&A...535L..11A). Our sample includes 19 thin disc stars and 130 thick disc stars with both N and O measurements. Their stellar parameters and the abundances of N and O are listed in tablea1.dat. (2 data files). ...File in questo prodotto:
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