Fig. 12
Download original image
Posterior distribution (dark blue) of the stellar rotation rate of TOI-815 after 150 Myr derived by PASTA. The solid black line represents the distribution of the stellar rotation rate of young open cluster stars with masses comparable to that of TOI-815 based on the collection of data provided by Johnstone et al. (2015a). The dashed black line indicates the observed present-day stellar rotation rate.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.