HST Observations of High-Density Globular Clusters
Abstract
In this paper we present preliminary results from our HST project aimed at exploring the connection between the stellar dynamics and stellar evolution in the cores of high-density globular clusters. We illustrate the discovery of horizontal branches (HB) with extended blue tails in the very metal rich globular clusters NGC 6388 ([Fe/H]=-0.6) and NGC 6441 ([Fe/H]=-0.5), and of a four-mode horizontal branch in NGC 2808. We briefly summarize the possible causes of these anomalies, which might be a signature of mass-loss processes,subtle composition variations, or dynamical effects. The existence of blue HBs in metal rich clusters and of significant narrow gaps between clumps on the HB are a challenge for the theoretical models. The composite color-magnitude diagram and luminosity function of 878 blue stragglers in our sample of 13 galactic globular clusters are also presented and briefly discussed.
Cite
@article{arxiv.astro-ph/9701152,
title = {HST Observations of High-Density Globular Clusters},
author = {G. Piotto and C. Sosin and I. R. King and S. G. Djorgovski and R. M. Rich and B. Dorman and A. Renzini and S. Phinney and J. Liebert},
journal= {arXiv preprint arXiv:astro-ph/9701152},
year = {2007}
}
Comments
8 pages, 1 Latex file, 7 Postscript Figures, 3 style files (epsf.sty, cupconf.sty and psfig.tex). Available at higher resolution as anonymous ftp at ftp://obelix.pd.astro.it/pub/elba/piotto.tar.gz To appear in: Advances in Stellar Evolution, ed. R. T. Rood and A. Renzini, (Cambridge U. Press: Cambridge)