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Fig. 22
Fitting of the differential mass distributions of ATLASGAL clumps above 1000 M⊙ within 1 kpc over the range of galactocentric radii from 3 to 8 kpc gives similar power-law exponents, α. There is a slightly decreasing slope of α with increasing galactocentric radius out to ~7 kpc and an increasing slope to α = −1.3 at 8 kpc.
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