Evidence for An Intermediate - age , Metal - rich Population of Globular Clusters in NGC 4365

Abstract

We present spectroscopy for globular clusters (GCs) in the elliptical galaxy NGC 4365, obtained with the LRIS spectrograph on the Keck I telescope. Previous studies have shown that the optical color distribution of GCs in NGC 4365 lacks the bimodal structure that is common in globular cluster systems, showing only a single broad peak. Measurements of Balmer line indices (Hβ, Hγ and

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Cite this paper

@inproceedings{Larsen2002EvidenceFA, title={Evidence for An Intermediate - age , Metal - rich Population of Globular Clusters in NGC 4365}, author={S\oren Schytt Larsen and Jean P . Brodie}, year={2002} }