Evolutionary track of a star with M = 1M⊙ and Z = Z⊙. Even if the oldest MS isochrones are close to pre-MS isochrones, however, ρ⋆ in the MS is sensibly higher with respect to the pre-MS phase. As a consequence, the mean stellar density enables us to discard unlikely age values according to ρ⋆.
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.