Fig. 20
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Posterior distribution (blue line) of the stellar rotation rate of HD 3167 after 150 Myrs derived by PASTA. The purple area represents the highest posterior density (HPD) interval of the distribution. The black line represents the distribution of the stellar rotation rate of young open cluster stars with mass comparable to that of HD 3167 based on the collection of data provided by Johnstone et al. (2015).
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