A study of runaway stars originating in the Scorpius-Centaurus-Lupus association

Open Access

Table E.1.

Questionable runaway candidates. There are three stars in the sample with space velocities that are significantly larger than those of the other candidates.

Star	SigMA	Group age	N_enc	${\bar{s}}_{min}$ $Mathematical equation: $ \overline{s}_{\text{min}} $$	$t ({\bar{s}}_{min})$ $Mathematical equation: $ t(\overline{s}_{\text{min}}) $$	v_pec,3D	v_rad	Ref.
		[Myr]	[per 1000]	[pc]	[Myr]	[km/s]	[km/s]	v_rad
Cl^* NGC 2264 VAS 133	14	$15 . 3_{- 0.3}^{+ 0.6}$ $Mathematical equation: $ 15.3_{-0.3}^{+0.6} $$	171	2.05	6.04±0.75	108.79	120.60 ± 2.00	[b]
Cl^* NGC 2264 VAS 133	8	$14 . 7_{- 0.7}^{+ 0.8}$ $Mathematical equation: $ 14.7_{-0.7}^{+0.8} $$	168	4.65	6.09±0.75	110.44	120.60 ± 2.00	[b]

Gaia DR3 4096398244806369792	17	$20 . 9_{- 0.8}^{+ 0.7}$ $Mathematical equation: $ 20.9_{-0.8}^{+0.7} $$	197	1.47	5.36±0.84	231.28	221.33 ± 26.69	[a]
Gaia DR3 4096398244806369792	21	$15 . 5_{- 0.5}^{+ 0.6}$ $Mathematical equation: $ 15.5_{-0.5}^{+0.6} $$	185	0.93	5.62±0.88	234.60	221.33 ± 26.69	[a]
Gaia DR3 4096398244806369792	10	$15 . 0_{- 1.4}^{+ 0.9}$ $Mathematical equation: $ 15.0_{-1.4}^{+0.9} $$	167	1.57	4.85±0.54	231.08	221.33 ± 26.69	[a]

Gaia DR3 4111239113458529152	5	$10 . 0_{- 0.5}^{+ 1.0}$ $Mathematical equation: $ 10.0_{-0.5}^{+1.0} $$	200	4.18	2.18±0.11	641.88	635.55 ± 8.26	[a]
Gaia DR3 4111239113458529152	15	$16 . 9_{- 0.6}^{+ 0.9}$ $Mathematical equation: $ 16.9_{-0.6}^{+0.9} $$	198	10.67	2.32±0.14	643.18	635.55 ± 8.26	[a]

Notes. In all three cases, the main reason for these high velocities are the respective radial velocities, which are included in this table along with the corresponding references ([a]: Gaia DR3; [b]: Hourihane et al. 2023). Additionally, the last two of these are also outliers on the color-magnitude diagram. The status as good runaway stars of these candidates remains doubtful until more research is conducted.

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