To clump or not to clump - The impact of wind inhomogeneities on the optical and NIR spectroscopic analysis of massive OB stars

Open Access

Fig. 23

Comparison of the observed Balmer and Brackett lines in HD 15570 (black) and HD 14947 (red). Whereas the Balmer lines are very similar, the Brackett lines Br₁₀ and Br₁₁ are much shallower in HD 14947. See text.

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