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

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Table H.2.

Photometric data of the three questionable runaway candidates.

Star	SpT	π [mas]	G_BP − G_RP	m_G [mag]	A_G [mag]	M_G [mag]
Cl* NGC 2264 VAS 133	B9v	1.76±0.20	0.3563	10.1584	0.8743±0.0042	$0 . 5062_{- 0.2618}^{+ 0.2343}$ $Mathematical equation: $ 0.5062_{-0.2618}^{+0.2343} $$
Gaia DR3 4096398244806369792	-	0.71±0.11	1.2264	12.8916	2.4663±0.0111	$- 0 . 3124_{- 0.3887}^{+ 0.3331}$ $Mathematical equation: $ -0.3124_{-0.3887}^{+0.3331} $$
Gaia DR3 4111239113458529152	-	0.61±0.04	1.5315	15.0641	2.9180±0.0178	$1 . 0666_{- 0.1584}^{+ 0.1574}$ $Mathematical equation: $ 1.0666_{-0.1584}^{+0.1574} $$

Notes. Spectral types (SpT) are taken from Skiff (2014, see references therein). For all stars in this table, parallaxes π, color indices G_BP − G_RP, apparent magnitudes m_G and extinction parameters A_G were taken from Gaia DR3.

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