{ "id": "1809.04350", "version": "v1", "published": "2018-09-12T10:29:31.000Z", "updated": "2018-09-12T10:29:31.000Z", "title": "Mergers, tidal interactions, and mass exchange in a population of disc globular clusters", "authors": [ "Sergey Khoperskov", "Alessandra Mastrobuono-Battisti", "Paola Di Matteo", "Misha Haywood" ], "comment": "13 pages, 9 figures, 6 embedded animations (for Acrobat only); high resolution movies available at https://goo.gl/YC546A; accepted by A&A", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "We present the results of a self-consistent $N$-body simulation following the evolution of a primordial population of thick disc globular clusters (GCs). We study how the internal properties of such clusters evolve under the action of mutual interactions, while they orbit a Milky Way-like galaxy. For the first time, through analytical and numerical considerations, we find that physical encounters between disc GCs are a crucial factor that contributed to the shape of the current properties of the Galactic GC system. Close passages or motion on similar orbits may indeed have a significant impact on the internal structure of clusters, producing multiple gravitationally bound sub-populations through the exchange of mass and even mergers. Our model produces two major mergers and a few small mass exchanges between pairs of GCs. Two of our GCs accrete stars from two companions, ending up with three internal sub-populations. We propose these early interactions and mergers between thick disc GCs with slightly different initial chemical compositions as a possible explanation for the presence of the spreads in metallicity observed in some of the massive Milky Ways GCs.", "revisions": [ { "version": "v1", "updated": "2018-09-12T10:29:31.000Z" } ], "analyses": { "keywords": [ "tidal interactions", "multiple gravitationally bound sub-populations", "thick disc globular clusters", "disc gcs", "small mass exchanges" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }