Omega Centauri, A Unique Window into Astrophysics

By F. V. Leeuwen, J. Hughes, G. Piotto. 2002

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Analysis of the Quiescent Low-Mass X-Ray Binary Population in Galactic Globular Clusters (2003, background): “Many sources outside the half-mass radius of ω Cen may be CVs, two of them brighter than LX = 10 32 ergs s−1 (Cool et al. 2002, Gendre et al. 2003).”
First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters (2003, methodology): “Using the age/turnoff mass relationship, the Kaluzny et al. (2002) analysis of this system yielded an age for this binary of 11.8 ± 0.6 Gyr.”
Super-Helium-rich Populations and the Origin of Extreme Horizontal-Branch Stars in Globular Clusters (2005, unknown): “ar X iv :a st ro -p h/ 05 01 50 0v 1 2 4 Ja n 20 05 Received 2004 December 23; accepted 2005 January 20 Preprint typeset using LATEX style emulateapj v. 6/22/04 evolution — stars: horizontal-branch”
A Deep Chandra Survey of the Globular Cluster 47 Tucanae: Catalog of Point Sources (2005, unknown): “Cen (Cool et al. 2002; Gendre et al. 2003), which has not yet dynamically relaxed.”
NEW LIMITS ON AN INTERMEDIATE-MASS BLACK HOLE IN OMEGA CENTAURI. II. DYNAMICAL MODELS (2009, methodology): “Third, Anderson (2002) studied luminosity functions (LFs) at different radii in ω Centauri using data obtained with HST.”