Formation of Omega Centauri From an Ancient Nucleated Dwarf Galaxy in the Young Galactic Disc
We first present a self-consistent dynamical model in which ω Cen is formed from an ancient nucleated dwarf galaxy merging with the first generation of the Galactic thin disc in a retrograde manner with respect to the Galactic rotation. Our numerical sim
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
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