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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.

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