New Limits on an Intermediate Mass Black Hole in Omega Centauri: II. Dynamical Models

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

28 pages, 11 figures, ApJ in press. v2 includes additions in response to referee comments

Scientific paper

10.1088/0004-637X/710/2/1063

We present a detailed dynamical analysis of the projected density and kinematical data available for the globular cluster Omega Cen. We solve the spherical anisotropic Jeans equation to predict the projected profiles of the RMS velocity in each of the three orthogonal coordinate directions (line of sight, proper motion radial, and proper motion tangential). We fit the models to new HST star count and proper motion data near the cluster center presented in Paper I, combined with existing ground-based measurements. We also derive and model the Gauss-Hermite moments of the observed proper motion distributions. The projected density profile is consistent with being flat near the center, with an upper limit gamma=0.07 on the central logarithmic slope. The RMS proper motion profile is also consistent with being flat near the center, and there are no unusually fast-moving stars. The models provide a good fit and yield a 1-sigma upper limit MBH < 1.2E4 solar masses on the mass of a possible intermediate-mass black hole (IMBH). The inferred upper limit corresponds to MBH/Mtot < 0.43%. We combine this with results for other clusters and discuss the implications for globular cluster IMBH demographics. Tighter limits will be needed to rule out or establish whether globular clusters follow the same black hole demographics correlations as galaxies. The arguments put forward by Noyola et al. (2008) to suspect an IMBH in Omega Cen are not confirmed by our study; the IMBH mass they suggested is firmly ruled out.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

New Limits on an Intermediate Mass Black Hole in Omega Centauri: II. Dynamical Models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with New Limits on an Intermediate Mass Black Hole in Omega Centauri: II. Dynamical Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New Limits on an Intermediate Mass Black Hole in Omega Centauri: II. Dynamical Models will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-450940

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.