The Globular Cluster Luminosity Function
arXiv:astro-ph/0302284 · doi:10.1007/10857603_50
Abstract
The main aspects of the globular cluster luminosity function needing to be explained by a general theory of cluster formation are reviewed, and the importance of simultaneously understanding globular cluster systematics (the fundamental plane) within such a theory is pointed out.
7 pages, to appear in Proceedings of the ESO Workshop on Extragalactic Globular Cluster Systems, ed. M. Kissler-Patig
References in corpus (1)
Cited by in corpus (5)
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- From young massive star cluster to old globular: the L_V-sigma_0 relationship as a diagnostic tool
- The old globular cluster system of the dIrr galaxy NGC1427A in the Fornax cluster