A Sequoia stellar candidate with very high 7Li and 9Be

Open Access

Fig. 3.

Observed spectrum (solid black) compared to the best fit (solid red) with A(Li) = 3.0. The UVES Li I 670.78 nm region of BPM 3066 is shown in the top panel. The Li Iλλ 610.36 nm 2²P-3²D subordinate transition is shown in the bottom panel; the strong line on the blue side is the Ca I 610.2723 nm line.

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