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 Image Credit: PanSTARRS DR1, PS1 Science Consortium |
The CMD is based on data kindly provided to us by Sylie Beaulieu
Observations
Cluster distance
Proper motion
Radial velocity
Orbit over the last 500 Myr
Velocity dispersion profile
Rotation
Color magnitude diagram
HST photometry
Mass function
MF slope
N-body Fits
Surface density
Proper motions
Radial velocities
Remnant fraction
Mass-to-light ratio
