A study of newly discovered close binary open cluster candidates in the Milky Way from Gaia DR3

Open Access

Fig. 6

Comparison of tidal radii obtained by HR23 (r_t23) and Tarricq et al. (2022) (r_t22) for 202 clusters. The tidal radius errors are taken from Tarricq et al. (2022). The blue line shows the isoline, and the red line shows a linear fit to the correlation.

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