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DENSITY AND KINEMATIC CUSPS IN M54 AT THE HEART OF THE SAGITTARIUS DWARF GALAXY: EVIDENCE FOR A 104 M BLACK HOLE?

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R. Ibata1, M. Bellazzini2, S. C. Chapman3, E. Dalessandro4, F. Ferraro4, M. Irwin3, B. Lanzoni4, G. F. Lewis5, A. D. Mackey6, P. Miocchi4 and A. Varghese1

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We report the detection of a stellar density cusp and a velocity dispersion increase in the center of the globular cluster M54, located at the center of the Sagittarius dwarf galaxy (Sgr). The central line-of-sight velocity dispersion is 20.2 ± 0.7 km s-1, decreasing to 16.4 ± 0.4 km s-1 at 2farcs5 (0.3 pc). Modeling the kinematics and surface density profiles as the sum of a King model and a point-mass yields a black hole mass of ~9400 M . However, the observations can alternatively be explained if the cusp stars possess moderate radial anisotropy. A Jeans analysis of the Sgr nucleus reveals a strong tangential anisotropy, probably a relic from the formation of the system.


Keywords

black hole physics; globular clusters: individual (M54); stellar dynamics


PACS

98.62.Js Galactic nuclei (including black holes), circumnuclear matter, and bulges

98.10.+z Stellar dynamics and kinematics

98.20.Jp Globular clusters in external galaxies

98.62.Lv Stellar content and populations; radii; morphology and overall structure

98.52.Wz Dwarf galaxies (elliptical, irregular, and spheroidal)

Subjects

Astrophysics and astroparticles

Dates

Issue 2 (2009 July 10)

Received 2009 April 21, accepted for publication 2009 June 2

Published 2009 June 25



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