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Chemical Abundance Analysis of Tucana III, the Second r-process Enhanced Ultra-Faint Dwarf Galaxy
[article]
2018
arXiv
pre-print
We present a chemical abundance analysis of four additional confirmed member stars of Tucana III, a Milky Way satellite galaxy candidate in the process of being tidally disrupted as it is accreted by the Galaxy. Two of these stars are centrally located in the core of the galaxy while the other two stars are located in the eastern and western tidal tails. The four stars have chemical abundance patterns consistent with the one previously studied star in Tucana III: they are moderately enhanced in
arXiv:1812.01022v1
fatcat:rkcleds33bfsxo7ajqja5pkvpy