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

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Table H.1.

Photometric data of the runaway candidates.

Star	SpT	π [mas]	G_BP − G_RP	m_G [mag]	A_G [mag]	Ref. A_G	M_G [mag]
λ CMa	B4v	7.41±0.11	-0.2241	4.4270	0.0002±0.0002	[1]	$- 1 . 2247_{- 0.0319}^{+ 0.0314}$ $Mathematical equation: $ -1.2247_{-0.0319}^{+0.0314} $$
HD 160093	B9iii	2.16±0.02	0.2612	9.3713	0.7503±0.0025	[1]	$0 . 2902_{- 0.0246}^{+ 0.0245}$ $Mathematical equation: $ 0.2902_{-0.0246}^{+0.0245} $$
66 Eri	B9.5(v)	10.73±0.11	-0.0710	5.0856	0.0069±0.0037	[1]	$0 . 2312_{- 0.0282}^{+ 0.0257}$ $Mathematical equation: $ 0.2312_{-0.0282}^{+0.0257} $$
γ Gru	B7iv	15.45±0.67	-0.0613	3.0000	0.0100	[2]	$- 1 . 0654_{- 0.0962}^{+ 0.0922}$ $Mathematical equation: $ -1.0654_{-0.0962}^{+0.0922} $$
γ Crv	B5/7	19.78±0.81	-0.0953	2.5800	0.0400	[2]	$- 0 . 9789_{- 0.0908}^{+ 0.0872}$ $Mathematical equation: $ -0.9789_{-0.0908}^{+0.0872} $$
α² CVn	B7v	29.60±1.04	-0.1072	2.8900	0.1150	[3]	$0 . 1315_{- 0.0777}^{+ 0.0750}$ $Mathematical equation: $ 0.1315_{-0.0777}^{+0.0750} $$
β Lib	B7.5iv	17.62±0.16	-0.0424	2.6100	0.0800	[2]	$- 1 . 2400_{- 0.0200}^{+ 0.0197}$ $Mathematical equation: $ -1.2400_{-0.0200}^{+0.0197} $$
ζ Oph	O9.2ivnn	8.91±0.20	0.1109	2.5400	0.8200	[4]	$- 3 . 5306_{- 0.0493}^{+ 0.0482}$ $Mathematical equation: $ -3.5306_{-0.0493}^{+0.0482} $$

Notes. All spectral types (SpT) are taken from Skiff (2014, see references therein). For the first three 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. For the rest of the stars, apparent magnitudes were retrieved from HIPPARCOS. For γ Crv and α² CVn, parallaxes were taken from the HIPPARCOS catalog and in the cases of γ Gru, β Lib and ζ Oph, the parallax values from van Leeuwen (2007) were used. Their G_BP − G_RP colors were converted from their B − V indices from HIPPARCOS as described above. The references of the extinction parameters are: [1]: Gaia DR3; [2]: Gontcharov (2012); [3]: Ghazaryan et al. (2018); [4]: Maiz Apellaniz & Barba (2018).

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