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arxiv: astro-ph/0211030 · v1 · submitted 2002-11-02 · 🌌 astro-ph

Spectroscopy of a Globular Cluster in the Local Group dIrr NGC 6822

classification 🌌 astro-ph
keywords clusterglobulargrouplocalclustersdirrspectroscopyviii
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We present low-resolution Keck spectroscopy for the globular cluster H VIII in the Local Group dIrr galaxy NGC 6822. We find the metallicity of the cluster to be [Fe/H]= -1.58 +/- 0.28 and the age of the cluster to be 3-4 Gyr, slightly older than but consistent with previous age estimates. H VIII seems to be more metal-poor than most intermediate-age globular clusters in the Local Group, and appears most similar to the anomalous Small Magellanic Cloud clusters Lindsay 113 and NGC 339.

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