Spectroscopic analysis of 348 red giants. II. (Adamow+, 2014)
This work is based on the Hobby-Eberly Telescope spectra obtained with the High Resolution Spectrograph, which we use for determination of abundances and rotational velocities. The Li abundance was determined from the 7Li 670.8nm line, while a more extended set of lines was used for alpha-elements abundances. Spectral analysis was done with the
Adamow, M. et al.
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2014