{ "id": "1007.4559", "version": "v1", "published": "2010-07-26T20:12:43.000Z", "updated": "2010-07-26T20:12:43.000Z", "title": "VLT Kinematics for omega Centauri: Further Support for a Central Black Hole", "authors": [ "Eva Noyola", "Karl Gebhardt", "Markus Kissler-Patig", "Nora Lutzgendorf", "Behrang Jalali", "P. Tim de Zeeuw", "Holger Baumgardt" ], "comment": "5 pages, published in The Astrophysical Journal Letters", "journal": "2010, ApJL, 719, L60", "categories": [ "astro-ph.GA" ], "abstract": "The Galactic globular cluster omega Centauri is a prime candidate for hosting an intermediate mass black hole. Recent measurements lead to contradictory conclusions on this issue. We use VLT-FLAMES to obtain new integrated spectra for the central region of omega Centauri. We combine these data with existing measurements of the radial velocity dispersion profile taking into account a new derived center from kinematics and two different centers from the literature. The data support previous measurements performed for a smaller field of view and show a discrepancy with the results from a large proper motion data set. We see a rise in the radial velocity dispersion in the central region to 22.8+-1.2 km/s, which provides a strong sign for a central black hole. Isotropic dynamical models for omega Centauri imply black hole masses ranging from 3.0 to 5.2x10^4 solar masses depending on the center. The best-fitted mass is 4.7+-1.0x10^4 solar masses.", "revisions": [ { "version": "v1", "updated": "2010-07-26T20:12:43.000Z" } ], "analyses": { "keywords": [ "central black hole", "proper motion data set", "vlt kinematics", "globular cluster omega centauri", "imply black hole masses" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/719/1/L60", "journal": "The Astrophysical Journal", "year": 2010, "month": "Aug", "volume": 719, "number": 1 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 863138, "adsabs": "2010ApJ...719L..60N" } } }