The intermediate neutron-capture process and carbon-enhanced metal-poor stars

Carbon-enhanced metal-poor (CEMP) stars in the Galactic Halo display enrichments in heavy elements associated with either the s (slow) or the r (rapid) neutron-capture process (e.g., barium and europium, respectively), and in some cases they display evidence of both. The abundance patterns of these...

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Bibliographic Details
Main Author: Hampel, Melanie (Author)
Format: Article (Journal)
Language:English
Published: 2016 November 10
In: The astrophysical journal
Year: 2016, Volume: 831, Issue: 2, Pages: 171
ISSN:1538-4357
DOI:10.3847/0004-637X/831/2/171
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/0004-637X/831/2/171
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Author Notes:Melanie Hampel, Richard J. Stancliffe, Maria Lugaro, and Bradley S. Meyer
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The intermediate neutron-capture process and carbon-enhanced metal-poor stars by Hampel, Melanie (Author)


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