{ "id": "1211.1889", "version": "v2", "published": "2012-11-08T16:01:05.000Z", "updated": "2013-05-18T23:15:29.000Z", "title": "Constraining the Statistics of Population III Binaries", "authors": [ "Athena Stacy", "Volker Bromm" ], "comment": "16 pages, 14 figures, to appear in MNRAS", "categories": [ "astro-ph.CO", "astro-ph.GA" ], "abstract": "We perform a cosmological simulation in order to model the growth and evolution of Population III (Pop III) stellar systems in a range of host minihalo environments. A Pop III multiple system forms in each of the ten minihaloes, and the overall mass function is top-heavy compared to the currently observed initial mass function in the Milky Way. Using a sink particle to represent each growing protostar, we examine the binary characteristics of the multiple systems, resolving orbits on scales as small as 20 AU. We find a binary fraction of ~36%, with semi-major axes as large as 3000 AU. The distribution of orbital periods is slightly peaked at < 900 yr, while the distribution of mass ratios is relatively flat. Of all sink particles formed within the ten minihaloes, ~50% are lost to mergers with larger sinks, and ~50% of the remaining sinks are ejected from their star-forming disks. The large binary fraction may have important implications for Pop III evolution and nucleosynthesis, as well as the final fate of the first stars.", "revisions": [ { "version": "v2", "updated": "2013-05-18T23:15:29.000Z" } ], "analyses": { "keywords": [ "population", "sink particle", "statistics", "initial mass function", "host minihalo environments" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/mnras/stt789", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2013, "month": "Aug", "volume": 433, "number": 2, "pages": 1094 }, "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1199248, "adsabs": "2013MNRAS.433.1094S" } } }