Fig. 6

Histogram of the extinction toward the stars detected in W3 Main with a bin size of 0.2 mag. Using the Nishiyama et al. (2009) extinction law, the stars are de-reddened in the CMD on to a 2 Myr main sequence and PMS isochrone. Changing the isochrone to 1 or 3 Myr does not change significantly the shape of the histogram. The solid line shows the histogram of the extinctions derived toward stars with JHKs detections, while the dashed line represents the extinction histogram of all the HKs sources (including the JHKs sources). The vertical dotted line denotes AKs = 0.4 mag and shows the division line between the foreground and the cluster population.
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