Fig. 3.
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Evolution of the orbital frequency (top panel), eccentricity (middle panel), and stellar angular momentum (bottom panel) as a function of system age obtained with TREMOR. Two initial stellar rotation rates were considered: Ωrot/Ωcrit = 0.2 and 0.3. The initial eccentricity was set to 0.1, and the initial orbital period of the system is 3.14 days.
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