{ "id": "1208.4851", "version": "v1", "published": "2012-08-23T20:00:06.000Z", "updated": "2012-08-23T20:00:06.000Z", "title": "N-body models of globular clusters: metallicity, half-light radii and mass-to-light ratios", "authors": [ "Anna C. Sippel", "Jarrod R. Hurley", "Juan P. Madrid", "William E. Harris" ], "comment": "14 pages, 10 figures, accepted for publication in MNRAS", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "Size differences of approx. 20% between red (metal-rich) and blue (metal-poor) sub-populations of globular clusters have been observed, generating an ongoing debate as to weather these originate from projection effects or the difference in metallicity. We present direct N-body simulations of metal-rich and metal-poor stellar populations evolved to study the effects of metallicity on cluster evolution. The models start with N = 100000 stars and include primordial binaries. We also take metallicity dependent stellar evolution and an external tidal field into account. We find no significant difference for the half-mass radii of those models, indicating that the clusters are structurally similar. However, utilizing observational tools to fit half-light (or effective) radii confirms that metallicity effects related to stellar evolution combined with dynamical effects such as mass segregation produce an apparent size difference of 17% on average. The metallicity effect on the overall cluster luminosity also leads to higher mass-to-light ratios for metal-rich clusters.", "revisions": [ { "version": "v1", "updated": "2012-08-23T20:00:06.000Z" } ], "analyses": { "keywords": [ "globular clusters", "mass-to-light ratios", "half-light radii", "n-body models", "metallicity effect" ], "tags": [ "journal article" ], "publication": { "doi": "10.1111/j.1365-2966.2012.21969.x", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2012, "month": "Nov", "volume": 427, "number": 1, "pages": 167 }, "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1181728, "adsabs": "2012MNRAS.427..167S" } } }