Mass and wind luminosity of young Galactic open clusters in Gaia DR2

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Table 1.

Comparison of our estimates of mass (second column) and the values provided by other works (fourth column) for a subset of clusters.

Cluster	M_c	T_age	M_c	T_age	Ref.
	[10³ M_⊙]	[Myr]	[10³ M_⊙]	[Myr]
Wd 1	22.2	7.9	49	4.0 ± 0.5	[1]
Danks 2	7.8	1.0	3.0 ± 0.8	$3 . 0_{- 1.0}^{+ 3.0}$ $3.0^{+3.0}_{-1.0}$	[2]
NGC 3603	4.8	1.0	13 ± 3	1−2	[3]
Danks 1	4.4	1.0	8.0 ± 1.5	$1 . 5_{- 0.5}^{+ 1.5}$ $1.5^{+1.5}_{-0.5}$	[2]
NGC 6231	3.2	13.8	3.75 ± 0.45	2–7	[4]
Wd 2	2.2	4.0	3.6	2.5	[5]
NGC 6611	1.7	2.14	25	2−5	[5]

Notes. The cluster ages are also reported, namely the values we considered from Gaia/MWSC catalog (third column) and the values usually adopted in the literature (fifth column).

References. The references are indicated in the last column and correspond to [1] = Gennaro et al. (2011); [2] = Davies et al. (2012); [3] = Harayama et al. (2008); [4] = Kuhn et al. (2017); [5] = Pfalzner (2009).

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