{ "id": "1501.01040", "version": "v1", "published": "2015-01-05T23:53:37.000Z", "updated": "2015-01-05T23:53:37.000Z", "title": "The emerging state of open clusters upon their violent relaxation", "authors": [ "Mario Spera", "Roberto Capuzzo-Dolcetta" ], "comment": "8 pages, 9 figures", "categories": [ "astro-ph.GA" ], "abstract": "The state after virialization of a small-to-intermediate N-body system depends on its initial conditions; in particular, systems that are, initially, dynamically \"cool\" (virial ratios Q=2T/|Omega| below ~ 0.3) relax violently in few crossing times. This leads to a metastable system (virial ratio ~ 1) which carries a clear signature of mass segregation much before the gentle 2-body relaxation time scale. This result is obtained by a set of high precision N-body simulations of isolated clusters composed of stars of two different masses (in the ratio m_h/m_l=2), and is confirmed also in presence of a massive central object (simulating a black hole of stellar size). We point out that this (quick) mass segregation occurs in two phases: the first one shows up in clumps originated by sub-fragmentation before the deep overall collapse; this segregation is erased during the deep collapse to re-emerge, abruptly, during the second phase that occurs after the first bounce of the system. This way to segregate masses, actual result of a violent relaxation, is an interesting feature also on the astronomical-observational side. In those stellar systems that start their dynamical evolution from cool conditions, this kind of mass segregation adds to the sequent, slow, secular segregation as induced by 2- and 3- body encounters.", "revisions": [ { "version": "v1", "updated": "2015-01-05T23:53:37.000Z" } ], "analyses": { "keywords": [ "violent relaxation", "open clusters", "emerging state", "virial ratio", "small-to-intermediate n-body system depends" ], "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2015arXiv150101040S" } } }