Fig. 9
Relation between the bolometric luminosity and the extinction-corrected ISOGAL (left) and MSX (right) flux densities at 15 μm for the YOs in our test sample. The error bars correspond to the standard deviations of the bolometric luminosity values. The slopes of the fitted lines are (4447 ± 106) L⊙/Jy (left) and (3736 ± 209) L⊙/Jy (right), respectively.
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