HST/ACS colour–magnitude diagrams of M 31 globular clusters

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Table 6:

Parameters derived for the candidate young clusters.
ID	$R_{\rm h}$	V	(B-V)	E(B-V)	Age	E (B-V)	Age
	(arcs)				(Myr)		(Myr)
				(this paper)		(C09)
B049-G112	1.20	17.56	0.52	0.30	280	0.25	400
B090	0.47	18.80					old
B367-G292	0.94	18.45	0.32	0.25	200	0.25	200
B458-D049	1.60	17.84	0.49	0.25	320	0.25	500
B515	1.25	18.60¹
B521-SK034A	0.75	19.08¹		0.55	400	0.38	250
M039	0.62	18.94		0.10	320	0.18	320
M050	0.80	18.71		0.15	560	0.25	300
B057-G118	0.70	17.64	0.69				old

Photometry is from G04 except when otherwise stated. $R_{\rm h}$ indicates the half-light radius.
¹: V magnitude from C09.

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