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Table 2.
Disentangled orbital parameters of UU Cas.
Solution | 1 | 2 | 3 | 4 | 5 | 6 | 7 |
Data | OAN | OAN | OAN | KAO | RNAO | AIO | GAO+APO |
Region | 5860–5884 | 5860–5884 | 5860–5884 | 5860–5884 | 5860–5884 | 5860–5884 | 5860–5884 |
Td | 2.314 ± 0.010 | 2.315 ± 0.007 | 2.335 ± 0.004 | 2.393 ± 0.004 | 2.314 ± 0.010 | 2.360 ± 0.005 | 2.429 ± 0.015 |
Kd | 191.5 ± 1.4 | 191.6 ± 1.0 | 186.6 ± 0.8 | 192.1 ± 0.5 | 200.6 ± 2.0 | 170.9 ± 0.8 | 192.5 ± 1.8 |
Q | 1.85 ± 0.04 | 2.25 ± 0.03 | 2.63 ± 0.24 | 2.26 ± 0.04 | 2.98 ± 0.21 | ||
Kg | < 0.1 | −8.4 ± 2.2 | 100.7 ± 1.9 | 85.4 ± 1.0 | 76.2 ± 7.0 | 75.5 ± 1.2 | 64.5 ± 4.4 |
σ | 0.0198 | 0.0197 | 0.0149 | 0.0246 | 0.0106 | 0.0284 | 0.0186 |
Solution | 8 | 9 | 10 | 11 | 12 | 13 | 14 |
Data | All | OAN | AIO | all | OAN,KAO,AIO | OAN | OAN |
Region | 5860–5884 | 6662–6691 | 6662–6691 | 6662–6691 | 7054–7078 | 4462–4486 | 4990–5031 |
Td | 2.391 ± 0.006 | 2.298 ± 0.007 | 2.297 ± 0.003 | 2.325 ± 0.008 | 2.319 ± 0.009 | 2.063 ± 0.008 | 2.300 ± 0.010 |
Kd | 187.6 ± 0.9 | 190.2 ± 1.1 | 187.0 ± 0.4 | 194.1 ± 1.1 | 195.2 ± 1.7 | 198.0 ± 2.0 | 197.0 ± 1.6 |
Q | 2.81 ± 0.10 | 2.11 ± 0.04 | 2.08 ± 0.02 | 3.39 ± 0.18 | 3.56 ± 0.19 | 2.29 ± 0.05 | 3.32 ± 0.17 |
Kg | 66.9 ± 2.4 | 90.1 ± 1.6 | 90.1 ± 0.9 | 57.3 ± 3.0 | 54.9 ± 2.9 | 86.6 ± 1.9 | 59.4 ± 3.0 |
σ | 0.0249 | 0.0196 | 0.0213 | 0.0226 | 0.0253 | 0.0276 | 0.0162 |
Solution | 15 | 16 | 17 | 18 | 19 | 20 | Mean |
Data | OAN | OAN | OAN | OAN | AIO | KAO | all |
Region | 5656–5690 | 4312–4365 | 4840–4889 | 6540–6607 | 6540–6607 | 6540–6580 | |
Td | 2.266 ± 0.014 | 2.063 ± 0.007 | 2.366 ± 0.009 | 2.503 ± 0.036 | 2.457 ± 0.016 | 2.280 ± 0.007 | 2.319 ± 0.087 |
Kd | 196.8 ± 2.0 | 193.4 ± 1.1 | 189.6 ± 1.7 | 129.7 ± 6.2 | 155.8 ± 2.9 | 169.7 ± 2.2 | 191.0 ± 7.4 |
Q | 2.63 ± 0.04 | 2.96 ± 0.14 | 2.32 ± 0.14 | 2.71 ± 0.09 | 3.34 ± 0.08 | 2.54 ± 0.68 | |
Kg | 73.5 ± 1.2 | 64.1 ± 3.0 | 55.9 ± 4.4 | 57.5 ± 1.9 | 50.8 ± 1.3 | 75.6 ± 14.4 | |
σ | 0.0152 | 0.0307 | 0.0193 | 0.0223 | 0.0224 | 0.0340 |
Notes. Td means HJD–2443130 of the eclipse of donor; Kd, Kg semiamplitudes in km s−1 of the RV-curves of the donor and gainer, respectively (note that Kg is suppressed by the circumstellar component in the two-component Solutions 1 and 2); Q mass ratio; σ residual noise.
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