arXiv · astro-ph/0211030
Spectroscopy of a Globular Cluster in the Local Group dIrr NGC 6822
Abstract
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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Jay Strader, Jean P. Brodie, John P. Huchra. 2002-11-02. Spectroscopy of a Globular Cluster in the Local Group dIrr NGC 6822. https://doi.org/10.1046/j.1365-8711.2003.06212.x
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