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Fig. 8

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Distributions of mass, surface density, temperature, luminosity, and luminosity-to-mass ratio as a function of the distance to the NVSS sources in the G29-SFR cloud. The NVSS number (Tables 5 and 6) is indicated in the lefthand upper corner of the upper panels. The dotted line in the surface density distributions indicates the minimum value needed needed to form massive stars according to theory (Butler & Tan 2012). The first bin contains only one point and, thus, the standard deviation is zero.

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