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Table 1

Star sample and photometric/spectroscopic data.

Star HD 156292 HD 24431 HD 105627 HD 116852 HD 153426 HD 218195 HD 36861 A HD 115455 HD 135591
(λ Orionis A)
Spec. type O9.7III O9III O9III O8.5II-III((f)) O8.5III O8.5III Nstr O8III O8III((f)) O8IV((f))

Spec. bin. SB2 SB2 SB2

Member. NGC 6322 Sh 2-205 Sh 2-2 Cep OB1 Sh 2-264 RCW 75 ASCC 79
Cam OB1 Collinder 69 Cen OB1
Ori OB1

Johnson U 7.101 6.507 7.270 8.380 6.650 7.657 2.196 7.400 (a) 4.442

Johnson B 7.773 7.117 8.182 8.380 7.610 8.650 3.218 8.170 (a) 5.372

Johnson V 7.509 6.745 8.140 8.470 7.470 8.357 3.405 7.970 (a) 5.457

Johnson R 6.360 (a)

Johnson I 6.100 (a)

2MASS J 6.944 5.917 7.985 8.720 7.057 7.755 3.735 (b) 7.469 5.554

2MASS H 6.886 5.826 8.030 8.789 7.056 7.708 3.769 (b) 7.442 5.566

2MASS Ks 6.855 5.839 8.069 8.795 7.027 7.735 3.876 (b) 7.454 5.616

E(BV) 0.52 0.63 0.30 0.17 0.40 0.55 0.07 0.46 0.17

Dist. (pc) 22 726−12 766
2857−1956 (c)

SWP № 16 218 30 166 20 623 09332 01517 26 975 46 234 16 087 48 294
07827-28 46 237
07828 46 241
46 245
46 247

SWP date 1982-Jan-31 1987-Jan-26 1983-Aug-06 1980-Jun-20 1978-May-10 1985-Oct-24 1992-Nov-12 1982-Jan-21 1993-Aug-03
1980-Jan-31 1992-Nov-12
1980-Jan-31 1992-Nov-12
1992-Nov-12
1992-Nov-12

LWP № 10 024 16 537 15 610 06841 06987 15 311 25 759

LWP date 1987-Jan-26 1983-Aug-06 1989-May-27 1980-Feb-02 1985-Oct-25 1989-Apr-05 1993-Jun-17

Vis. inst. FEROS ESPADONS FEROS FEROS FEROS ESPADONS NARVAL FEROS FEROS

Vis. date 2016-Mar-23 2011-Nov-07 2016-Mar-18 2016-Mar-18 2016-Mar-18 2011-Jul-05 2007-Sep-21 2016-Mar-18 2016-Mar-18

Notes. Spectral types, spectroscopic binary classification, and memberships are from Sota et al. (2014). Photometric data are from Maíz-Apellániz et al. (2004) with exception to the specific references. Color excesses are calculated considering intrinsic colors calibrated by spectral type from Martins & Plez (2006). Distances are from Gaia Collaboration (2018). For HD36861, we adopted the distance from the mean Gaia DR2 parallaxes for the components C and D, as in Gordon et al. (2018). Distance from van Leeuwen (2007) for HD 116852 is shown too. All distances are obtained from the direct inversion of the measured parallaxes. We list information about the analyzed data in the UV (SWP and LWP number and observation date) and in the visible (instrument name/observation date) regions.

References. (a) Ducati (2002). (b) Cutri et al. (2003). (c)van Leeuwen (2007).

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