Abstract
We report on new observations of the globular cluster systems (GCSs) of two galaxies: M86 (NGC 4406) in Virgo and NGC 4696, the central giant elliptical (gE) in the Centaurus cluster. Previous observations in M86 showed no evidence for bimodality, but using only (V — I) for small cluster samples. The NGC 4696 GCS is unstudied. We used the integrated Washington (C —T 1) color. This metallicity index is more than twice as sensitive to [Fe/H] as (V — I). In M86 we have about 1100 good GC candidates, and about 650 in NGC 4696, with mean internal metallicity errors ∼ 0.15 dex. Both of these GCSs are found to have bimodal metallicity distributions (MDs). Our data strengthen previous results that MDs for the GCSs of gEs are widespread. The evidence for 2 separate populations in these galaxies is corroborated by examining the surface density distributions: the metal-rich clusters are more centrally concentrated than their metal-poor counterparts. The overall radial metallicity gradient present in the M86 GCS is due to the varying radial mix of the 2 populations. The existence of 2 GC populations signifies that there were 2 distinct epochs or events of cluster formation in a gE. The simple collapse model of gE formation is ruled out.
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© 1999 Springer Science+Business Media Dordrecht
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Geisler, D., Lee, M.G. (1999). Multimodal Color Distributions in the Globular Cluster Systems of Giant Elliptical Galaxies. In: Barnes, J.E., Sanders, D.B. (eds) Galaxy Interactions at Low and High Redshift. International Astronomical Union, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4665-4_45
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DOI: https://doi.org/10.1007/978-94-011-4665-4_45
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-5833-6
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