Fig. 8
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Posterior distribution (dark blue) of the stellar rotation rate of HD 190622 after 150 Myr derived by PASTA. The purple area represents the HPD interval of the distribution. The black line represents the distribution of the stellar rotation rate of young open cluster stars with masses comparable to that of HD 190622 based on the collection of data provided by Johnstone et al. (2015). See main text for details.
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