A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models

Open Access

Fig. A.2.

Same as in Fig. A.1, but for our binary models with an initial orbital period of P_i = 10 d and an initial mass ratio of q_i = 0.5. In contrast to Fig. A.1, the optical depths here mark fixed values of the wind optical depths in the range from τ = 1.5 − 3.5 and are labeled accordingly.

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