Fig. 13.
Mean equatorial velocity during the MS as a function of LZAMS, the total angular momentum content at the ZAMS. The two curves show 20 M⊙ models computed at solar metallicity (red) and at Z = 10−5 (blue, the models of Table 2). The two peaks of the Huang & Gies (2006, H+2006) and Ramírez-Agudelo et al. (2013, Ra+2013) velocity distributions are indicated, together with the vv6 and vv7 models.
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