{ "id": "1007.3493", "version": "v1", "published": "2010-07-20T20:00:01.000Z", "updated": "2010-07-20T20:00:01.000Z", "title": "A Galactic Center Origin for HE 0437-5439, the Hypervelocity Star near the Large Magellanic Cloud", "authors": [ "Warren R. Brown", "Jay Anderson", "Oleg Y. Gnedin", "Howard E. Bond", "Margaret J. Geller", "Scott J. Kenyon", "Mario Livio" ], "comment": "5 pages, accepted in ApJ Letters", "journal": "Brown et al 2010, ApJ, 719, L23", "doi": "10.1088/2041-8205/719/1/L23", "categories": [ "astro-ph.GA" ], "abstract": "We use Hubble Space Telescope imaging to measure the absolute proper motion of the hypervelocity star (HVS) HE 0437-5439, a short-lived B star located in the direction of the Large Magellanic Cloud (LMC). We observe (\\mu_\\alpha, \\mu_\\delta)=(+0.53+-0.25(stat)+-0.33(sys), +0.09+-0.21(stat)+-0.48(sys)) mas/yr. The velocity vector points directly away from the center of the Milky Way; an origin from the center of the LMC is ruled out at the 3-sigma level. The flight time of the HVS from the Milky Way exceeds its main-sequence lifetime, thus its stellar nature requires it to be a blue straggler. The large space velocity rules out a Galactic-disk ejection. Combining the HVS's observed trajectory, stellar nature, and required initial velocity, we conclude that HE 0437-5439 was most likely a compact binary ejected by the Milky Way's central black hole.", "revisions": [ { "version": "v1", "updated": "2010-07-20T20:00:01.000Z" } ], "analyses": { "keywords": [ "large magellanic cloud", "galactic center origin", "hypervelocity star", "vector points directly away", "milky ways central black hole" ], "tags": [ "journal article" ], "publication": { "journal": "The Astrophysical Journal", "year": 2010, "month": "Aug", "volume": 719, "number": 1 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 862159, "adsabs": "2010ApJ...719L..23B" } } }