A two-dimensional perspective of the rotational evolution of rapidly rotating intermediate-mass stars - Implications for the formation of single Be stars

Open Access

Fig. 4.

Average value of the equatorial velocity with respect to the critical one, ⟨V_eq/V_c⟩, divided by the initial value at the ZAMS, as a function of stellar mass. Data points in grey show the observationally derived upper limits of V_eq/V_c taken from the last column of Table 7 of Huang et al. (2010).

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