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 Image Credit: VVV DR5, ESO, Institute for Astrophysics, ROE |
The CMD is based on data kindly provided to us by Edouardo Lagioia
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
