R. Ibata et al 2009 ApJ 699 L169 doi:10.1088/0004-637X/699/2/L169
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
Show affiliationsWe 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 2
5 (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.
black hole physics; globular clusters: individual (M54); stellar dynamics
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)
Issue 2 (2009 July 10)
Received 2009 April 21, accepted for publication 2009 June 2
Published 2009 June 25
R. Ibata et al 2009 ApJ 699 L169
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C B Muratov and V V Osipov 2000 J. Phys. A: Math. Gen. 33 8893
G Allen et al 2006 J. Phys.: Conf. Ser. 32 117
S Higuchi et al 2006 J. Phys.: Conf. Ser. 32 125
Serdar Kuyucak et al 2001 Rep. Prog. Phys. 64 1427
M Donszelmann et al 2008 J. Phys.: Conf. Ser. 119 032016