Fig. 14
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Comparison between the properties of GLOSTAR H II regions that are associated with ATLASGAL dust clumps (in red) and those that are not linked to ATLASGAL clumps (in blue). CDFs are presented for various properties of GLOSTAR H II regions. The results of the Anderson-Darling (AD) tests, indicated above each plot, provide insights into the statistical significance of the observed differences.
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