The R-process alliance: discovery of the first metal-poor star with a combined r- and s-process element signature

We present a high-resolution (R ∼ 35,000), high signal-to-noise ratio (S/N > 200) Magellan/MIKE spectrum of the star RAVE J094921.8-161722, a bright (V = 11.3) metal-poor red giant star with [Fe/H] = -2.2, identified as a carbon-enhanced metal-poor (CEMP) star from the RAVE survey. We report its...

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Bibliographic Details
Main Authors: Gull, Maude (Author), Frebel, Anna (Author), Cain, Madelyn G. (Author), Ji, Alexander P. (Author), Ezzeddine, Rana (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: American Astronomical Society, 2020-04-07T02:29:32Z.
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