Kinematics of Tidal Debris from ω Centauri’s Progenitor Galaxy

@article{Mizutani2003KinematicsOT,
  title={Kinematics of Tidal Debris from $\omega$ Centauri’s Progenitor Galaxy},
  author={Arihiro Mizutani and Masashi Chiba and Tsuyoshi Sakamoto},
  journal={The Astrophysical Journal},
  year={2003},
  volume={589}
}
We present the kinematic properties of a tidally disrupted dwarf galaxy in the Milky Way, based on the hypothesis that its central part once contained the most massive Galactic globular cluster, ω Cen. Dynamical evolution of a self-gravitating progenitor galaxy that follows the present-day and likely past orbits of ω Cen is calculated numerically and the kinematic nature of their tidal debris is analyzed, combined with randomly generated stars comprising spheroidal halo and flat disk components… 
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