Free Access
Fig. 2
Polar magnetic strength of an exoplanet that is required to ensure a certain probability to retain its atmosphere when it orbits a saturated star at the boundaries of the HZ as a function of stellar mass.
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.