**Table 5:** Comparison of [DBS2003] 179 with other young, massive clusters. The compilation data are from Brandner et al. (2008, Table 9). The footnotes list the sources for the data on each individual cluster.
	Wd1^a	ONC^b	Wd2^c	NGC 3603YC^d	Arches^e	R136 cluster^f	[DBS2003] 179
Age [Myr]	$3.6\pm0.7$	0.3-1.0	1-3	2.5	2-3	2-3	2.5-5
$t_{\rm relax}$ [Myr]	400	2.1		10-40	2?		7
$r_{\rm hm}$ [pc]	1.0	0.8		0.7-1.5	0.24	1.1	0.2
$N_{\rm tot}$	10⁵	>2800		$1.6\times 10^4$	>3450		>1240
$M_{\rm tot}$ [ $M_{\odot}$ ]	$5\times 10^4$	$0.18\times 10^4$	$0.7\times10^4$	1- $1.6\times 10^4$	> $1.3 \times 10 ^4$	$10 \times 10 ^4$	$(0.7--0.8) \times 10^4$

^a Brandner et al. (2008); ^b Hillenbrand & Hartmann (1998); ^c Ascenso et al. (2007); ^d Harayama et al. (2007); ^e Figer et al. (1999); Stolte et al. (2005); ^f Andersen et al. (2007); Brandl et al. (1999).

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