Stellar Populations in Globular Cluster Cores: Evidence for a Peculiar Trend Among Red Giant Branch Stars
arXiv:0909.2864 · doi:10.1111/j.1745-3933.2009.00749.x
Abstract
We investigate the relationship between the mass of a globular cluster core and the sizes of its various stellar populations in a sample of 56 globular clusters. The number of core red giant branch stars is found to scale sub-linearly with core mass at the 3- confidence level, whereas the relation is linear to within one standard deviation for main-sequence turn-off and sub-giant branch stars. We interpret our results as evidence for a surplus of red giant branch stars in the least massive cluster cores which is not seen for main-sequence turn-off and sub-giant branch stars. We explore various possibilities for the source of this discrepancy, discussing our results primarily in terms of the interplay between the cluster dynamics and stellar evolution.
5 pages, 2 figures, accepted by MNRAS Letters
References in corpus (9)
- The fraction of binary systems in the core of thirteen low-density Galactic globular clusters
- A Binary Origin for Blue Stragglers in Globular Clusters
- NGC 6441: another indication for a very high helium content in Globular Cluster stars
- On the structure of tidal tails
- Blue Stragglers After the Main Sequence
- The chemical evolution of Omega Centauri's progenitor system
- NGC2298: a globular cluster on its way to disruption
- Evolved Stars in the Core of the Massive Globular Cluster NGC 2419
- On the radial distribution of horizontal branch stars in ngc2808
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- On the origins of enigmatic stellar populations in Local Group galactic nuclei
- Dissecting the Colour-Magnitude Diagram: A Homogeneous Catalogue of Stellar Populations in Globular Clusters