Deep ACS Imaging in the Globular Cluster NGC 6397: The Cluster Color Magnitude Diagram and Luminosity Function

Abstract

We present the CMD from deep HST imaging in the globular cluster NGC 6397. The ACS was used for 126 orbits to image a single field in two colors (F814W, F606W) 5 arcmin SE of the cluster center. The field observed overlaps that of archival WFPC2 data from 1994 and 1997 which were used to proper motion (PM) clean the data. Applying the PM corrections produces a remarkably clean CMD which reveals a number of features never seen before in a globular cluster CMD. In our field, the main sequence stars appeared to terminate close to the location in the CMD of the hydrogen-burning limit predicted by two independent sets of stellar evolution models. The faintest observed main sequence stars are about a magnitude fainter than the least luminous metal-poor field halo stars known, suggesting that the lowest luminosity halo stars still await discovery. At the bright end the data extend beyond the main sequence turnoff to well up the giant branch. A populous white dwarf cooling sequence is also seen in the cluster CMD. The most dramatic features of the cooling sequence are its turn to the blue at faint magnitudes as well as an apparent truncation near F814W = 28. The cluster luminosity and mass functions were derived, stretching from the turn off down to the hydrogen-burning limit. It was well modeled with either a very flat power-law or a lognormal function. In order to interpret these fits more fully we compared them with similar functions in the cluster core and with a full N-body model of NGC 6397 finding satisfactory agreement between the model predictions and the data. This exercise demonstrates the important role and the effect that dynamics has played in altering the cluster IMF.

43 pages including 4 tables and 12 diagrams. Figures 2 and 3 have been bitmapped. Accepted for publication in the Astronomical Journal

References in corpus (5)

• The ACS Survey of Galactic Globular Clusters. I. Overview and Clusters Without Previous HST Photometry
• The core binary fractions of star clusters from realistic simulations
• Probing the Faintest Stars in a Globular Star Cluster
• Halo Stars Near the Hydrogen-Burning Limit: The M/L Subdwarf Transition
• Deep ACS Imaging in the Globular Cluster NGC6397: Dynamical Models

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• Solar-like oscillations in a metal-poor globular cluster with the HST
• Investigating the age and structure of the infrared old open clusters LK1, LK10, FSR1521 and FSR1555
• Deep ACS Imaging in the Globular Cluster NGC6397: Dynamical Models
• Constraining white-dwarf kicks in globular clusters : II. Observational Significance
• Optical and Near-Infrared Spectroscopy of the L Subdwarf SDSS J125637.13-022452.4