Journal article
Dynamical evolution and spatial mixing of multiple population globular clusters
Monthly notices of the Royal Astronomical Society, v 429(3), pp 1913-1921
01 Mar 2013
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Abstract
Numerous spectroscopic and photometric observational studies have provided strong evidence for the widespread presence of multiple stellar populations in globular clusters. In this paper, we study the long-term dynamical evolution of multiple population clusters, focusing on the evolution of the spatial distributions of the first-(FG) and second-generation (SG) stars. In previous studies, we have suggested that SG stars formed from the ejecta of FG AGB stars are expected initially to be concentrated in the cluster inner regions. Here, by means of N-body simulations, we explore the time-scales and the dynamics of the spatial mixing of the FG and the SG populations and their dependence on the SG initial concentration.
Our simulations show that, as the evolution proceeds, the radial profile of the SG/FG number ratio, N-SG/N-FG, is characterized by three regions: (1) a flat inner part; (2) a declining part in which FG stars are increasingly dominant and (3) an outer region where the N-SG/N-FG profile flattens again (the N-SG/N-FG profile may rise slightly again in the outermost cluster regions). Until mixing is complete and the N-SG/N-FG profile is flat over the entire cluster, the radial variation of N-SG/N-FG implies that the fraction of SG stars determined by observations covering a limited range of radial distances is not, in general, equal to the SG global fraction, (N-SG/N-FG)(glob). The distance at which N-SG/N-FG equals (N-SG/N-FG)(glob) is approximately between 1 and 2 cluster half-mass radii. The time-scale for complete mixing depends on the SG initial concentration, but in all cases complete mixing is expected only for clusters in advanced evolutionary phases, having lost at least 60-70 per cent of their mass due to two-body relaxation (in addition to the early FG loss due to the cluster expansion triggered by SNII ejecta and gas expulsion). The results of our simulations suggest that in many Galactic globular clusters the SG should still be more spatially concentrated than the FG.
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Details
- Title
- Dynamical evolution and spatial mixing of multiple population globular clusters
- Creators
- Enrico Vesperini - Indiana UniversityStephen L. W. McMillan - Drexel UniversityFrancesca D'Antona - National Institute for AstrophysicsAnnibale D'Ercole - Osservatorio astronomico di Bologna
- Publication Details
- Monthly notices of the Royal Astronomical Society, v 429(3), pp 1913-1921
- Publisher
- Oxford Univ Press
- Number of pages
- 9
- Grant note
- grant PRIN-INAF; Ministry of Education, Universities and Research (MIUR); Research Projects of National Relevance (PRIN)
- Resource Type
- Journal article
- Language
- English
- Academic Unit
- Physics
- Web of Science ID
- WOS:000318271300006
- Scopus ID
- 2-s2.0-84874041380
- Other Identifier
- 991019167531904721
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- Collaboration types
- Domestic collaboration
- International collaboration
- Web of Science research areas
- Astronomy & Astrophysics