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Table 1

Stellar properties.

CX Dra π Aqr ϕ Per

Spec. type B2.5Ve+F5III B1Ve+[A-F] B2[e]+sdO
M1 [M] 3.9 14.0 ± 1.0 9.3 ± 0.3
M2 [M] 0.9 2.3 1.1 ± 0.1
Porb [d] 6.696 84.1 127
D [pc] 396 ± 35 240 ± 15 220 ± 9
z [pc] 149 169 43
nH [cm-3] 0.45 0.37 1.30
RV [km s-1] −2.1 ± 2.3 −4.9 ± 0.1 −4.0 ± 2.1

v [km s-1] 21.1 ± 2.0 21.0 ± 1.1 29.8 ± 1.6
PA [°] 107.6 ± 1.2 82.3 ± 0.6 119.7 ± 0.2
i [°] −5.7 ± 63.1 −13.5 ± 1.2 −7.7 ± 30.3

v∗ ,LSR [km s-1] 25.5 ± 2.1 13.5 ± 1.0 13.1 ± 1.7
PALSR [°] 125.7 ± 1.0 31.5 ± 0.5 109.4 ± 0.6
iLSR [°] 32.4 ± 11.4 6.6 ± 3.7 −4.4 ± 90

Ref. 1 2, 3, 4 5

Notes. The space velocities were calculated following Johnson & Soderblom (1987) using the Hipparcos proper motion and parallax (van Leeuwen 2007) and radial velocities from the catalogue by de Bruijne & Eilers (2012). The solar motion adopted to convert heliocentric motion into LSR motion is (U,V,W) = (8.50 ± 0.29, 13.38 ± 0.43, 6.49 ± 0.26) km s-1 (Coşkunoǧlu et al. 2011).

Reference. (1) Berdyugin & Piirola (2002); (2) Zharikov et al. (2013); (3) Linnell et al. (1988); (4) Bjorkman et al. (2002); (5) Hummel & Štefl (2001).

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