Chemical abundances of metal-poor RR Lyrae stars in the Magellanic Clouds

We present for the first time a detailed spectroscopic study of chemical element abundances of metal-poor RR Lyrae stars in the Large and Small Magellanic Cloud (LMC and SMC). Using the MagE echelle spectrograph at the 6.5 m Magellan telescopes, we obtain medium resolution (R ~ 2000-6000) spectra of...

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Detalhes bibliográficos
Principais autores: Haschke, Raoul, Grebel, Eva K., Frebel, Anna L.
Outros Autores: Massachusetts Institute of Technology. Department of Physics
Formato: Artigo
Idioma:en_US
Publicado em: IOP Publishing 2013
Acesso em linha:http://hdl.handle.net/1721.1/76331
https://orcid.org/0000-0002-2139-7145