Quantifying the contamination by old main-sequence stars in young moving groups: the case of the Local Association

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Table 1:

Young moving groups.
Moving group	Age [Myr]	Associated cluster(s)
Local Association	10-300	Pleiades, $\alpha$ Per, M34,
		$\delta$ Lyr, NGC 2516, IC 2602
IC 2391 Supercluster	80-250	IC 2391
Castor	200	-
Ursa Major	300-500	Ursa Major
Hyades Supercluster	650	Hyades, Praesepe

Source LaTeX | All tables | In the text

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