Gaia DR3 reveals the complex dynamical evolution within star clusters

Open Access

Fig. 5.

$\bar{D_{i}}$ $\bar{D_{\mathrm{i}}}$ , $\bar{D_{c}}$ $\bar{D_{\mathrm{c}}}$ and $\bar{D_{cc}}$ $\bar{D_{\mathrm{cc}}}$ (kpc) vs. distance for our sample of ∼1500 open clusters color-coded by their PC1 value. The black dashed vertical line represents the slope change location. The solid yellow and blue lines are a linear fit to the data at both intervals of slope change point.

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