Figure 6: (a) Distribution of radio luminosity, , with bolometric luminosity, , for YSOs (figure reproduced from ); (b) distribution of radio detected YSOs as a function of bolometric luminosity, compared to the expected distribution of YSOs from Dunham and Vorobyov . Grey hatching indicates objects from the combined catalogues of Anglada , Furuya et al. , and Scaife et al. [151–153]. Red hatching indicates the objects detected at 16 GHz [151–153].