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Table 3

Components in α and δ of the vector r1, which provides the position of the barycenter or center of luminosity with respect to the position of the primary star for the close binary systems in UX Ari, HD 283447, and DoAr51.

Barycenter Center of luminosity Difference
r1,α* σr1,α* r1,δ σr1,δ r1,α* σr1,α* r1,δ σr1,δ r1,α* σr1,α* r1,δ σr1,δ
UX Ari, P 1 −0.707 0.020 −0.139 0.052 −0.304 0.009 −0.060 0.022 −0.403 0.022 −0.079 0.056
UX Ari, P 2 −0.708 0.019 −0.111 0.049 −0.305 0.008 −0.048 0.021 −0.403 0.021 −0.063 0.053
HD 283447, P 1 1.286 0.045 0.873 0.111 0.568 0.020 0.386 0.049 0.717 0.049 0.487 0.121
HD 283447, P 2 1.283 0.045 0.924 0.113 0.567 0.020 0.408 0.050 0.716 0.050 0.515 0.123
DoAr51, P 1 −2.003 0.052 −2.795 0.153 −2.169 0.057 −3.028 0.166 0.167 0.077 0.233 0.226

Notes. If two primary calibrators – P 1 and P 2 – were available for phase-referencing, the results from referencing to each of them are shown. The standard deviations for the components of the vector r1, and , are based on random error (see Sect. 3.2) and variance propagation. Units are in milliarcseconds.

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