The velocity field of the Scorpius-Centaurus OB association - I. Method and general properties

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Table A.1

Overview of the clusters in the main selection.

SigMA name	N_stars	age [Myr]
Antares	502	${12.7}_{- 1.3}^{+ 0.4}$ $12.7_{ - 1.3}^{ + 0.4}$
ρ Sco	240	${13.7}_{- 0.6}^{+ 1.3}$ $13.7_{ - 0.6}^{ + 1.3}$
Scorpio-Body	373	${14.7}_{- 0.7}^{+ 0.8}$ $14.7_{ - 0.7}^{ + 0.8}$
US-foreground	276	${19.1}_{- 1.3}^{+ 2.4}$ $19.1_{ - 1.3}^{ + 2.4}$
V1062-Sco	1029	${15.0}_{- 1.4}^{+ 0.9}$ $15.0_{ - 1.4}^{ + 0.9}$
µ Sco	54	${17.2}_{- 2.4}^{+ 0.9}$ $17.2_{ - 2.4}^{ + 0.9}$
Libra-South	71	${20.0}_{- 2.2}^{+ 2.5}$ $20.0_{ - 2.2}^{ + 2.5}$
η Lup	769	${15.3}_{- 0.3}^{+ 0.6}$ $15.3_{ - 0.3}^{ + 0.6}$
ϕ Lup	1114	${16.9}_{- 0.6}^{+ 0.9}$ $16.9_{ - 0.6}^{ + 0.9}$
e Lup	516	${20.9}_{+ 0.8}^{+ 0.7}$ $20.9_{ + 0.8}^{ + 0.7}$
UPK606	131	${13.4}_{- 0.7}^{+ 1.0}$ $13.4_{ - 0.7}^{ + 1.0}$
ρ Lup	246	${14.4}_{- 0.9}^{+ 0.4}$ $14.4_{ - 0.9}^{ + 0.4}$
ν Cen	1737	${15.7}_{- 0.9}^{+ 0.3}$ $15.7_{ - 0.9}^{ + 0.3}$
σ Cen	1805	${15.5}_{- 0.5}^{+ 0.6}$ $15.5_{ - 0.5}^{ + 0.6}$
Acrux	394	${11.2}_{- 1.0}^{+ 1.0}$ $11.2_{ - 1.0}^{ + 1.0}$
Musca-foreground	95	${10.2}_{- 0.7}^{+ 1.0}$ $10.2_{ - 0.7}^{ + 1.0}$
ϵ Cham	39	${8.8}_{- 0.4}^{+ 0.6}$ $8.8_{ - 0.4}^{ + 0.6}$
η Cham	30	${9.4}_{- 0.9}^{+ 1.4}$ $9.4_{ - 0.9}^{ + 1.4}$
Pipe-North	42	${15.9}_{- 2.1}^{+ 1.6}$ $15.9_{ - 2.1}^{ + 1.6}$
θ Oph	98	${15.4}_{- 1.9}^{+ 0.8}$ $15.4_{ - 1.9}^{ + 0.8}$
CrA-Main	96	${8.5}_{- 2.4}^{+ 2.0}$ $8.5_{ - 2.4}^{ + 2.0}$
CrA-North	351	${11.6}_{- 0.6}^{+ 0.5}$ $11.6_{ - 0.6}^{ + 0.5}$
Scorpio-Sting	132	${14.5}_{- 0.6}^{+ 0.6}$ $14.5_{ - 0.6}^{ + 0.6}$
Centaurus-Far	99	${8.5}_{- 1.3}^{+ 1.1}$ $8.5_{ - 1.3}^{ + 1.1}$
Chamaeleon-1	192	${3.8}_{- 0.9}^{+ 1.9}$ $3.8_{ - 0.9}^{ + 1.9}$
Chamaeleon-2	54	${2.8}_{- 0.9}^{+ 0.7}$ $2.8_{ - 0.9}^{ + 0.7}$
L134/L183	24	${9.6}_{- 2.2}^{+ 1.7}$ $9.6_{ - 2.2}^{ + 1.7}$

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