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HST Observations of the Globular Cluster M4
Published online by Cambridge University Press: 25 May 2016
Abstract
The WFPC2 aboard the Hubble Space Telescope has been used to obtain deep images in three fields at different radial positions in the nearest Globular cluster, M4 (NGC 6121). In this paper, we discuss the white dwarf cooling sequence and show how the dynamical structure of the cluster will affect their cumulative distribution function. We also present the first discussion of our observations of the faint cluster main sequence stars.
- Type
- New Observations with HST
- Information
- Symposium - International Astronomical Union , Volume 174: Dynamical Evolution of Stars Clusters , 1996 , pp. 39 - 48
- Copyright
- Copyright © Kluwer 1996