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Fig. 11


Comparison of the strength and shape of the [Ca II] λ 7291 and the Ca II λλ 8498, 8542, 8662 emission lines seen in the du Pont data and in FEROS spectra from 2014 and 2015. The Ca II triplet lines are blended with the Paschen lines Pa16, Pa15 and Pa13, respectively.

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