NLTE corrections to europium abundances in metal-poor stars are small and line-dependent, and do not require significant changes to r-process parameters in galactic chemical evolution models.
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NLTE abundances of Eu for a sample of metal-poor stars in the Galactic Halo and Metal-poor Disk with 1D and <3D> models
NLTE corrections to europium abundances in metal-poor stars are small and line-dependent, and do not require significant changes to r-process parameters in galactic chemical evolution models.