Fig. 11
IMF of the γ Velorum cluster. The dotted line is the IMF derived from the sample of confirmed and possible members of γ Velorum observed with GIRAFFE while the thick solid line is the IMF corrected for incompleteness. The overplotted dashed segments represent the Kroupa (2001) IMF to which we applied an arbitrary vertical shift, while the solid segments show the IMF obtained with our fit.
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.