Chemical Abundances of New Member Stars in the Tucana II Dwarf Galaxy

Chemical Abundances of New Member Stars in the Tucana II Dwarf Galaxy

We present chemical abundance measurements for seven stars with metallicities ranging from Fe/H] =-3.3 to [Fe/H] =-2.4 in the Tucana II ultra-faint dwarf galaxy (UFD), based on high-resolution spectra obtained with the MIKE spectrograph on the 6.5 m Magellan-Clay Telescope. For three stars, we prese...

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Bibliographic Details
Main Authors: Ji, Alexander P. (Author), Jerjen, Helmut (Author), Kim, Dongwon (Author), Norris, John E. (Author), Chiti, Anirudh (Contributor), Frebel, Anna L. (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: American Astronomical Society, 2018-08-27T18:07:16Z.
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