A photometric study of NGC 458
arXiv:astro-ph/9610104
Abstract
We present a CCD investigation of the poorly known SMC young Globular Cluster NGC 458. The NTT data, presented here, allowed us to study in detail the more internal regions of the cluster which are less contaminated by the field. On the basis of theoretical isochrones, a preliminary evaluation of the age is also given.
4 pages, 7 postscript figures; to appear in: Proceedings of the Elba Meeting ``Stellar Ecology'', ed. R.T. Rood