Chemical abundances in a high velocity RR Lyrae star near the bulge

Low-mass, variable, high-velocity stars are interesting study cases for many aspects of Galactic structure and evolution. Until recently, the only known high- or hyper-velocity stars were young stars thought to originate from the Galactic centre. Wide-area surveys like APOGEE and BRAVA have found se...

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Bibliographic Details
Main Authors: Hansen, Camilla Juul (Author) , Koch-Hansen, Andreas (Author) , Ludwig, Hans-Günter (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: March 21, 2016
In: Arxiv

Online Access:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1603.05654
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Author Notes:Camilla Juul Hansen, Robert Michael Rich, Andreas Koch, Siyi Xu, Andrea Kunder, Hans-Guenter Ludwig
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Chemical abundances in a high-velocity RR Lyrae star near the bulge by Hansen, Camilla Juul (Author) , Koch-Hansen, Andreas (Author) , Ludwig, Hans-Günter (Author) ,


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