THE CHEMICAL COMPOSITIONS OF VERY METAL-POOR STARS HD 122563 AND HD 140283: A VIEW FROM THE INFRARED

From high resolution (R sime 45,000), high signal-to-noise ratio (S/N > 400) spectra gathered with the Immersion Grating Infrared Spectrograph (IGRINS) in the H and K photometric bands, we have derived elemental abundances of two bright, well-known metal-poor halo stars: the red giant HD 122563 a...

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Bibliographic Details
Main Authors: Sneden, Christopher (Author), Kim, Hwihyun (Author), Mace, Gregory N. (Author), Kaplan, Kyle F. (Author), Lee, Hye-In (Author), Oh, Heeyoung (Author), Oh, Jae Sok (Author), Pak, Soojong (Author), Park, Chan (Author), Pavel, Michael D. (Author), Yuk, In-Soo (Author), Jaffe, Daniel T. (Author), Afsar, Melike (Author), 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: IOP Publishing, 2016-05-23T23:08:16Z.
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