Fig. 4.
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Star formation progression in Sco-Cen, shown with the same orientation in XYZ and color-scaling as in Fig. 1. By separating the clusters in age bins, following the peaks in Fig. 3 and Table 2, one can appreciate a consistent inside-out progression of star formation from older to younger clusters. For more details, see the interactive 3D version online or at https://homepage.univie.ac.at/sebastian.ratzenboeck/wp-content/uploads/2023/05/scocen_age.html.
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