Survival of protoplanetary disks in Upper Scorpius from population synthesis models with external photoevaporation

Open Access

Fig. 1

PDF of external FUV flux F_UV, fit with log-normal distribution. Light, medium, and dark blue lines represent 16th, median, and 84th values of the FUV flux in the Upper Sco star forming region, respectively. The red line enclosing the blue lines shows the distribution from which we draw FUV flux, F_UV, in our models.

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