The Flattening of Globular Clusters

Abstract

In the three nearest luminous galaxies, the Milky Way System, the Andromeda Galaxy and NGC 5128 the brightest globular clusters are rounder than the faintest ones. On the other hand (contrary to some previous results) the flattening of individual LMC clusters is found to be independent of their luminosities. This suggests the possibility that the relationship between the flattening and luminosity of clusters might depend on host galaxy luminosity. No significant differences are found between the intrinsic flattening distributions of Galactic old halo, Galactic young halo and Galactic bulge/disk clusters. Such a dependence might perhaps have been expected if tidal forces (which are largest at small Galactocentric distances) removed angular momentum from globular clusters. The preliminary conclusion by Norris that clusters with blue horizontal branches are more flattened than red HB clusters is not confirmed by the larger data base that is now available. In other words there is no evidence for the puzzling claimed correlation between the flattening and the horizontal branch morphology of Galactic globular clusters.

20 pages text + tables; 5 postscript figures. Astronomical Journal, in press

References in corpus (6)

• The properties of Galactic globular cluster sub-systems
• Structural parameters for globular clusters in M31 and generalizations for the fundamental plane
• Kinematic Decoupling of Globular Clusters with Extended Horizontal-Branch
• Structural Parameters for Globular Clusters in NGC 5128. II: HST/ACS Imaging and New Clusters
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