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. 6

Comparison between the stellar parameters obtained by Holgado (2019; see also Holgado et al. 2018) and our work. Upper left panel: effective temperature. The dashed lines represent ± 1000 K; upper right panel: logarithmic gravity (±0.1 dex); lower left panel: log Q (±0.2 dex); lower right panel: helium abundance Y_He(±0.03). Numbers indicate the stars as listed in Table 1.

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