Fig. 2.
DSS greyscale image centred on NGC 3603. North is up and east is to the left. The blue arrows show the predicted motions relative to NGC 3603 YC of RFS7 and RFS8, for a time-span of 0.4 Myr. The red lines in the opposite directions are proportional to the apparent age of the star, thus illustrating the site of potential origin. The magenta circles are centred on NGC 3603 YC with a radii 0.5′ (solid line) and 5′ (dashed line) indicating the approximate boundaries of NGC 3603 YC and NGC 3603, respectively.
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