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A Survey of Globular Cluster Velocity Dispersions
Published online by Cambridge University Press: 19 July 2016
Extract
We have used the Dominion Astrophysical Observatory radial velocity spectrometer on the 3.6m Canada-France-Hawaii telescope to obtain radial velocities, accurate to ~0.8 km/s, for ~20 stars in each of nine globular clusters. The stars are generally within three core radii of the cluster center. The cluster names and metallicities (the latter are averages of values in Zinn and West (1984), Pilachowski (1984), and Webbink (1985)) are given in Table I. This sample includes two clusters with cusps in their surface brightness profiles: NGC 6624 and 6681.
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- Chapter X. Poster Papers on Formation and Evolution of Globular Clusters
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- Copyright © Kluwer 1988