Simulations of Globular Cluster Evolution with Multiple Stellar Populations
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| Format: | Preprint |
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2025
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| _version_ | 1866912635890434048 |
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| author | Giersz, Mirek Askar, Abbas Hypki, Arkadiusz Hong, Jongsuk Wiktorowicz, Grzegorz Hellstrom, Lucas |
| author_facet | Giersz, Mirek Askar, Abbas Hypki, Arkadiusz Hong, Jongsuk Wiktorowicz, Grzegorz Hellstrom, Lucas |
| contents | The formation of stars with light-element abundance variations in globular clusters and the subsequent dynamical evolution of these multiple populations remains an open question. One of the most widely discussed is the AGB scenario, in which chemically processed material from the envelopes of AGB stars mixes with re-accreted primordial gas flowing into the center of the cluster. Based on this scenario, more than two hundred MOCCA simulations of cluster evolution have been carried out, incorporating additional physical processes related to the external environment of globular clusters and the initial properties of multiple stellar populations. Analysis of the simulations shows that most observed properties of multiple stellar populations and the global parameters of Milky Way clusters are well reproduced, with the exception of the correlation between cluster mass and the fraction of second-population stars. We present a speculative scenario of globular cluster evolution that may account for the observed properties of Milky Way clusters, including the correlation between cluster mass and the fraction of enriched stars. The scenario further predicts that, under certain conditions, the pristine first population can be more centrally concentrated than the enriched second population, as observed in some clusters. \end{abstract |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2510_06942 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Simulations of Globular Cluster Evolution with Multiple Stellar Populations Giersz, Mirek Askar, Abbas Hypki, Arkadiusz Hong, Jongsuk Wiktorowicz, Grzegorz Hellstrom, Lucas Astrophysics of Galaxies The formation of stars with light-element abundance variations in globular clusters and the subsequent dynamical evolution of these multiple populations remains an open question. One of the most widely discussed is the AGB scenario, in which chemically processed material from the envelopes of AGB stars mixes with re-accreted primordial gas flowing into the center of the cluster. Based on this scenario, more than two hundred MOCCA simulations of cluster evolution have been carried out, incorporating additional physical processes related to the external environment of globular clusters and the initial properties of multiple stellar populations. Analysis of the simulations shows that most observed properties of multiple stellar populations and the global parameters of Milky Way clusters are well reproduced, with the exception of the correlation between cluster mass and the fraction of second-population stars. We present a speculative scenario of globular cluster evolution that may account for the observed properties of Milky Way clusters, including the correlation between cluster mass and the fraction of enriched stars. The scenario further predicts that, under certain conditions, the pristine first population can be more centrally concentrated than the enriched second population, as observed in some clusters. \end{abstract |
| title | Simulations of Globular Cluster Evolution with Multiple Stellar Populations |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2510.06942 |