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Fig. 5

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Observed colors for stars in Westerlund 2, with data for the Wolf-Rayet stars WR 20a and WR 20b plotted as circled yellow points. The intrinsic relation for dwarfs is plotted as a solid black curve, with the same relation reddened by EB − V = 1.65 as a gray curve. Reddening lines of slope EU − B/EB − V = 0.64 are plotted relative to the hottest O stars and A3 dwarfs (red lines), and B5 dwarfs (blue line). A similar reddening line of slope EU − B/EB − V = 0.75 is shown for the hottest O stars (green line).

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