Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-09-02
Astrophysical Journal, 668, 139L (2007)
Astronomy and Astrophysics
Astrophysics
ApJ Letter in press
Scientific paper
10.1086/522927
We have used a combination of high resolution (HST ACS-HRC, ACS-WFC, and WFPC2) and wide-field (ESO-WFI) observations of the galactic globular cluster NGC 6388 to derive its center of gravity, projected density profile, and central surface brightness profile. While the overall projected profiles are well fit by a King model with intermediate concentration (c=1.8) and sizable core radius (rc=7"), a significant power law (with slope \alpha=-0.2) deviation from a flat core behavior has been detected within the inner 1 arcsecond. These properties suggest the presence of a central intermediate mass black hole. The observed profiles are well reproduced by a multi-mass isotropic, spherical model including a black hole with a mass of ~5.7x10^3 Msol.
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Dalessandro Emanuele
Ferraro Francesco R.
Lanzoni Barbara
Miocchi Paolo
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