0000000000430006
AUTHOR
S. Villanova
The Gaia-ESO Survey : Probes of the inner disk abundance gradient
The nature of the metallicity gradient inside the solar circle (R_GC < 8 kpc) is poorly understood, but studies of Cepheids and a small sample of open clusters suggest that it steepens in the inner disk. We investigate the metallicity gradient of the inner disk using a sample of inner disk open clusters that is three times larger than has previously been studied in the literature to better characterize the gradient in this part of the disk. We used the Gaia-ESO Survey (GES) [Fe/H] values and stellar parameters for stars in 12 open clusters in the inner disk from GES-UVES data. Cluster mean [Fe/H] values were determined based on a membership analysis for each cluster. Where necessary, dis…
CCDC 684060: Experimental Crystal Structure Determination
Related Article: S.Fustero, J.F.Sanz-Cervera, S.Merida, R.Roman, S.Villanova, C.R.de Arellano|2008|J.Fluorine Chem.|129|836|doi:10.1016/j.jfluchem.2008.04.004
CCDC 684059: Experimental Crystal Structure Determination
Related Article: S.Fustero, J.F.Sanz-Cervera, S.Merida, R.Roman, S.Villanova, C.R.de Arellano|2008|J.Fluorine Chem.|129|836|doi:10.1016/j.jfluchem.2008.04.004