The Most Metal-Poor Stars. IV. The Two Populations With [Fe/H] [< over ~] -3.0

The Most Metal-Poor Stars. IV. The Two Populations With [Fe/H] [< over ~] -3.0

We discuss the carbon-normal and carbon-rich populations of Galactic halo stars having [Fe/H] [< over ~] –3.0, utilizing chemical abundances from high-resolution, high signal-to-noise model-atmosphere analyses. The C-rich population represents ~28% of stars below [Fe/H] = –3.1, with the present C...

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Bibliographic Details
Main Authors: Frebel, Anna L., Norris, John E., Yong, David, Bessell, M. S., Christlieb, N., Asplund, M., Gilmore, Gerard, Wyse, Rosemary F. G., Beers, Timothy C., Barklem, P. S., Ryan, S. G.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2013
Online Access:http://hdl.handle.net/1721.1/76329
https://orcid.org/0000-0002-2139-7145

Internet

http://hdl.handle.net/1721.1/76329
https://orcid.org/0000-0002-2139-7145

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