How universal are the two young cluster sequences? - The cases of the LMC, SMC, M 83, and the Antennae

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Volume 508 / No 1 (December II 2009)

A&A, 508 1 (2009) L5-L8

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Table 2:

Properties of clusters younger than $\log (t_{\rm c})$ = 8.00 in the LMC.
Identifier	$\log (\rm age)$	$\Delta$ age	Radius	$\Delta$ radius	$M_{\rm total}$	$\Delta M_{\rm total}$	$\log (\rho)$	$\Delta \rho$
	[Myr]		[pc]		[ $M_{\odot }$ ]		[ $M_{\odot }$ /pc^-3]
NGC 1805¹	7.0	0.3	1.33	0.06	3.52	0.13	2.54	0.2
NGC 1818¹	7.4	0.3	2.45	0.09	4.13	0.15	2.35	0.2
NGC 1984¹	7.06	0.3	0.99	0.07	3.38	0.24	2.79	0.2
NGC 2004 ¹	7.30	0.2	1.57	0.13	4.43	0.38	2.32	0.2
NGC 2011¹	6.99	0.3	1.17	0.12	3.47	0.14	3.24	0.12
NGC 2100²	7.20	0.3	1.14	0.14	4.43	0.13	3.05	0.2
R 136¹	6.48	0.18	0.32	0.02	4.55	0.21	4.47	0.08

¹ Mackey & Gilmore (2003a); and ² McLaughlin & van der Marel (2006).

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