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A new look at globular cluster colors in NGC 3311 and the case for exclusively metal-rich globular cluster systems

Jean P. Brodie·Soeren S. Larsen·Markus Kissler-Patig
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Abstract

NGC 3311, the central cD galaxy in the Hydra cluster, was previously thought to host the most metal-rich globular cluster system known. Ground-based Washington photometry had indicated the almost complete absence of the population of globular clusters near [Fe/H] ~ -1 dex, normally dominant in the metallicity distribution functions of giant elliptical galaxies. Lacking the normal metal-poor globular cluster population, NGC 3311 was an outstanding exception among galaxies, not easily understood under any of the current globular cluster formation scenarios. Our HST/WFPC2 data yield normal globular cluster colors and hence metallicities for this galaxy. We find a bi-modal color distribution with peaks at (V-I)=0.91 +/- 0.03 and 1.09 +/- 0.03, corresponding to [Fe/H] ~ -1.5 and -0.75 dex (somewhat dependent on the choice of the conversion relation between color and metallicity). We review the evidence for exclusively metal-rich globular cluster systems in other galaxies and briefly discuss the implications for our understanding of globular cluster and galaxy formation.

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Jean P. Brodie, Soeren S. Larsen, Markus Kissler-Patig. 2000-08-22. A new look at globular cluster colors in NGC 3311 and the case for exclusively metal-rich globular cluster systems. https://doi.org/10.1086/318166

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