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Table · dataset · 2012

Abundances of M22 subgiants

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We present an abundance analysis of 101 subgiant branch (SGB) stars in the globular cluster M22.

Description

Using low-resolution FLAMES/GIRAFFE spectra we have determined abundances of the neutron-capture strontium and barium and the light element carbon. With these data we explore relationships between the observed SGB photometric split in this cluster and two stellar groups characterized by different contents of iron, slow neutron-capture process (s-process) elements, and the {alpha} element calcium, which we previously discovered in M22's red-giant stars.

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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/541/a1514 d agoJSON v1
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concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
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