Spectum of Be doublet

This image shows the region of the Be II doublet of the metal-poor stars LP815-43 (V = 10.91) and CD -24°17504 (V=12.18) in the reduced UVES -spectra, with Be and the other main features marked. The dotted lines are synthetic spectra computed with preliminary stellar parameters to aid the line identification. The model for LP 815-43 was computed with a tentative beryllium abundance of log(Be/H) + 12 = -1.3.