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Fig. 2
Synthetic PoWR spectra calculated for fixed parameters (T* = 50 kK, log L = 5.3 [L⊙], M = 13 M⊙, v∞ = 1000 km s−1, D = 10, surface hydrogen mass fraction XH = 0.4, LMC-like composition) but different Rt (see legend). The figure illustrates that stars with Rt values above a certain threshold would not appear as WR stars.
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