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Non-LTE Abundances in OB stars: Preliminary Results for 5 Stars in the Outer Galactic Disk

The aim of this study is to analyse and determine elemental abundances for a large sample of distant B stars in the outer Galactic disk in order to constrain the chemical distribution of the Galactic disk and models of chemical evolution of the Galaxy. Here, we present preliminary results on a few stars along with the adopted methodology based on securing simultaneous O and Si ionization equilibria with consistent NLTE model atmospheres.

preprint2014arXivOpen access
G. A. BragançaT. LanzS. DaflonK. CunhaC. D. GarmanyJ. W. GlaspeyM. Borges FernandesM. S. OeyT. BensbyI. Hubeny
astro-ph.SR
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Open access10 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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G. A. BragançaT. LanzS. DaflonK. CunhaC. D. GarmanyJ. W. GlaspeyM. Borges FernandesM. S. OeyT. BensbyI. Hubeny

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