Fig. 3.
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Evolution of the long model compared to simulations with a constant magnetic field strength. The initial stellar ages of the 1.0 and 0.7 M⊙ models are tinit = 2.0 and 5.0 Myr (see Table 1), respectively. Panel a: Accretion rate. Panel b: Truncation radius, rt, and the corotation radius, Rco, in units of the stellar radius. Panel c: Fastness parameter, ωS.
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