RACE-OC project: Rotation and variability of young stellar associations within 100 pc

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Table 10:

List of target associations/clusters, age, number of stars used to make the statistics, median and mean rotation period, and significance level that consecutive period distributions are drawn from the same distribution.
		0.6-1.2 $M_{\odot}$				0.8-1.2 $M_{\odot}$
Target	age	#	$P_{\rm median}$	$P_{\rm mean}$	KS	#	$P_{\rm median}$	$P_{\rm mean}$	KS
	(Myr)	stars	(d)	(d)		stars	(d)	(d)
ONC	1	33	6.83	6.17	0.57	16	6.83	5.93	0.70	1 vs. 4 Myr
NGC 2264	4	26	5.43	6.19	0.59	10	4.72	5.15	0.63	4 vs. 9 Myr
TW Hya + $\beta$ Pic	9	30	4.83	4.52	0.09	23	3.40	4.31	0.17	9 vs. 30 Myr
Tuc/Hor + Car + Col	30	62	2.85	3.22	0.36	53	2.60	2.87	0.45	30 vs. 70 Myr
$\alpha$ Persei	70	54	0.77	2.39	0.11	48	0.77	2.49	0.26	70 vs. 110 Myr
AB Dor + Pleiades	110	89	2.29	3.16	...	48	3.33	3.32	...	...

Source LaTeX | All tables | In the text

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