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Cited article:

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Radial anisotropy in ω Cen limiting the room for an intermediate-mass black hole

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Discovery of high-velocity EHB stars in the globular clusterωCentauri (NGC 5139)

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Research in Astronomy and Astrophysics 15 (10) 1639 (2015)
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SCIENTIFIC POTENTIAL OF DECIGO PATHFINDER AND TESTING GR WITH SPACE-BORNE GRAVITATIONAL WAVE INTERFEROMETERS

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Mass estimates from stellar proper motions: the mass of ω Centauri

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AnXMM-Newtonsearch for X-ray sources in the Fornax dwarf galaxy

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Astronomy & Astrophysics 550 A18 (2013)
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EVOLUTION OF SECOND-GENERATION STARS IN STELLAR DISKS OF GLOBULAR AND NUCLEAR CLUSTERS: ω CENTAURI AS A TEST CASE

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Gas depletion in primordial globular clusters due to accretion on to stellar-mass black holes

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THE VELOCITY DISPERSION PROFILE OF NGC 6388 FROM RESOLVED-STAR SPECTROSCOPY: NO EVIDENCE OF A CENTRAL CUSP AND NEW CONSTRAINTS ON THE BLACK HOLE MASS

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The Astrophysical Journal 769 (2) 107 (2013)
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A SEARCH FOR AN INTERMEDIATE-MASS BLACK HOLE IN THE CORE OF THE GLOBULAR CLUSTER NGC 6266

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Exploring intermediate and massive black-hole binaries with the Einstein Telescope

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