Fig. 7
LX/LBOL distribution as a function of LBOL. The three couples of lines refer to the (25%, 50%, 75%) quartiles of the LX/LBOL distributions calculated in running intervals of constituted by 80 contiguous points and smoothed in interval of bolometric luminosity of 0.1 erg s-1. The continuous line refer to Class II stars, and the dashed one to the Class III stars.
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