An in-depth spectroscopic examination of molecular bands from 3D hydrodynamical model atmospheres: II. Carbon-enhanced metal-poor 3D model atmospheres
Context. Tighter constraints on metal-poor stars we observe are needed to better understand the chemical processes of the early Universe. Computing a stellar spectrum in 3D allows one to model complex stellar behaviours, which cannot be replicated in 1D. Aims. We examine the effect that the intrinsi...
Gespeichert in:
| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
February 1, 2017
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| In: |
Arxiv
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| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1701.09102
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| Verfasserangaben: | A.J. Gallagher, E. Caffau, P. Bonifacio, H.-G. Ludwig, M. Steffen, D. Homeier, B. Plez |
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