Articulo
A double stellar generation in the globular cluster NGC 6656 (M 22). Two stellar groups with different iron and s-process element abundances
Astronomy & Astrophysics
Registro en:
15010003
15010003
Autor
Marino, A. F.
Villanova, S.
Institución
Resumen
We present a chemical abundance analysis based on high resolution UVES spectra of seventeen bright giant stars in the Globular Cluster (GC) M 22. We obtained an average iron abundance of [Fe/H] = -1.76±0.02 (internal errors only) and an α enhancement of 0 FONDAP FONDAP