SIMBAD references

2009A&A...508..695C - Astronomy and Astrophysics, volume 508, 695-706 (2009/12-3)

Intrinsic iron spread and a new metallicity scale for globular clusters.

CARRETTA E., BRAGAGLIA A., GRATTON R., D'ORAZI V. and LUCATELLO S.

Abstract (from CDS):

We have collected spectra of about 2000 red giant branch (RGB) stars in 19 Galactic globular clusters (GC) using FLAMESLT (about 100 stars with GIRAFFE and about 10 with UVES, respectively, in each GC). These observations provide an unprecedented, precise, and homogeneous data-set of Fe abundances in GCs. We use it to study the cosmic scatter of iron and find that, as far as Fe is concerned, most GCs can still be considered mono-metallic, since the upper limit to the scatter of iron is less than 0.05dex, meaning that the degree of homogeneity is better than 12%. The scatter in Fe we find seems to have a dependence on luminosity, possibly due to the well-known inadequacies of stellar atmospheres for upper-RGB stars and/or to intrinsic variability. It also seems to be correlated with cluster properties, like the mass, indicating a larger scatter in more massive GCs which is likely a (small) true intrinsic scatter. The 19 GCs, covering the metallicity range of the bulk of Galactic GCs, define an accurate and updated metallicity scale. We provide transformation equations for a few existing scales. We also provide new values of [Fe/H], on our scale, for all GCs in the Harris catalogue.

Abstract Copyright:

Journal keyword(s): stars: abundances - stars: atmospheres - stars: population II - globular clusters: general

Simbad objects: 136

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2009A&A...508..695C and select 'bookmark this link' or equivalent in the popup menu


2020.12.05-01:18:32

© Université de Strasbourg/CNRS

    • Contact