The Eddington factor as the key to understand the winds of the most massive stars - Evidence for a Γ-dependence of Wolf-Rayet type mass loss

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Fig. 4

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Under the assumption of central He-burning, the Arches cluster stars display no general Γ-dependence. Symbols are the same as in Fig. 3, the black dashed line indicates a fitted relation (Eq. (14)) for WNh stars (parameters from Table 2 row 3).

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