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Table 5.

Other properties used to compute the apsidal motion of the systems analysed.

System T0 ω0 r1 r2 v1 sin i v2 sin i i
[BJD] [deg] [km s−1] [km s−1] [deg]
KX Cnc 2456910.0768 63.76 0.01940(4) 0.01913(4) 6.4(1.0) 6.5(1.0) 89.825(3)
AL Dor 2458368.7277 107.45 0.0333(3) 0.0334(3) 4.6(1.0) 4.6(1.0) 88.79(11)
V541 Cyg 2450817.9760 262.72 0.0431(2) 0.0419(3) 15(1) 15(1) 89.83(3)
V459 Cas 2454815.5698 240.32 0.0726(3) 0.0710(3) 54(2) 43(2) 89.467(7)
V501 Her 2455648.5943 250.10 0.08375(11) 0.06323(11) 14.3(1.0) 12.5(1.0) 89.11(4)
KW Hya 2453430.9533 225.29 0.0853(5) 0.0594(8) 15(2) 13(2) 87.5(3)
V501 Mon 2458477.9808 232.79 0.0838(13) 0.0707(13) 16.5(1.0) 12.4(1.0) 88.02(8)
GG Ori 2451952.4777 122.89 0.0746(10) 0.0737(10) 24(2) 23(2) 89.30(10)
EY Cep 2458836.4248 110.14 0.0603(4) 0.0606(8) 10(1) 10(1) 89.89(3)

Notes. The table lists: the reference time and the corresponding argument of periastron, the stellar relative radii and projected rotational velocities, and the orbital inclination of the system.

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