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Table 3.

Orbital velocities, rotational velocities, and luminosities of the semi-detached double-lined eclipsing binaries, whenever available.

Name Period vrot, a sin i vrot, d sin i Ωrot, aorb Ωrot, dorb log La log Ld Inclination i
(d) (km s−1) (km s−1) (L) (L) (deg)
VFTS 061 2.33 174 152 1.18 1.02 4.77 ± 0.04 4.75 ± 0.05 69.1
MP Cen 2.99 140 95 1.07 0.85 3.80 ± 0.20 3.00 ± 0.20 82.2
LZ Cep 3.07 130 80 0.67 0.51 5.11 ± 0.19 4.69 ± 0.19 48.1
VFTS 538 4.15 158 108 2.24 0.82 4.96 ± 0.08 5.31 ± 0.06 47.0
XZ Cep 5.09 230 110 1.62 0.78 5.05 ± 0.06 4.79 ± 0.22 80.0
VFTS 450 6.89 380 97 4.44 0.66 5.30 ± 0.21 5.46 ± 0.04 63.5
VFTS 652 8.59 224 96 2.75 1.08 5.35 ± 0.06 4.92 ± 0.06 63.7
AQ Cas 11.70 287 98 4.94 0.96 4.94 ± 0.08 4.59 ± 0.05 84.4

Notes. The references to each individual system are the same as in Tables 1 and 2. The subscript ‘a’ denotes the accreting star and ‘d’ denotes the Roche lobe filling mass donating star.

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