Gaia DR3 reveals the complex dynamical evolution within star clusters

Open Access

Table A.1.

Main properties of the final sample of 81 open clusters used in this study.

Cluster	$\bar{D_{i}}$ $\bar{D_{i}}$ (kpc)	$\bar{D_{c}}$ $\bar{D_{c}}$ (kpc)	$\bar{D_{cc}}$ $\bar{D_{cc}}$ (kpc)	Age (Gyr)	R_gc (kpc)	ecc	Z_max (kpc)	PC1	PC2	PC3
ADS_16795	0.017	0.004	0.012	0.035	8.199	0.035	0.069	0.790	0.126	0.083
Alessi_9	0.004	0.001	0.003	0.257	7.918	0.060	0.059	0.585	0.234	0.181
CWNU_1010	0.006	0.002	0.004	0.079	8.254	0.049	0.082	0.580	0.294	0.126
CWNU_1015	0.008	0.002	0.006	0.040	8.265	0.059	0.047	0.531	0.404	0.065
CWNU_1018	0.011	0.002	0.007	0.135	8.251	0.048	0.161	0.700	0.191	0.109

Notes. Only a segment of this table is displayed here. A machine-readable version of the complete table is accessible at the CDS.

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