Table 9: The same as Table 8, for stars considered as non-members by us.
ID $_{\rm BDA}$ ID $_{\rm Zhao}$ $P_{\rm P}$ $P_{\rm NP}$ $P_{\rm c}$ Vr* ID $_{\rm BDA}$ ID $_{\rm Zhao}$ $P_{\rm P}$ $P_{\rm NP}$ $P_{\rm c}$ Vr*
8 822 0.00 0.70 3 29.1 $\pm$1.8 7116 27 0.00 0.00 3 13.7 $\pm$0.0
10 136 0.00 0.00 3 16.3 $\pm$0.0 7232 52 0.00 0.00 3 4.2 $\pm$0.0
45 857 0.00 0.00 3 -14.0 $\pm$0.0 7251 434 0.00 0.47 0 34.56$\pm$0.14 SB1
49 3 0.00 0.00 3 28.1 $\pm$0.0 7335 75 0.00 0.00 3 -18.9 $\pm$0.0
144 951 0.00 0.00 0 33.72$\pm$0.14 SB1 7350 72 0.00 0.00 3 -13.0 $\pm$0.0
155 943 0.00 0.00 3 3.6 $\pm$1.0 7378 458 0.00 0.00 3 57.8 $\pm$0.0
173 963 0.00 0.00 0 33.37$\pm$0.20 SB1 7434 94 0.00 0.65 0 33.7 $\pm$0.9
200 601 0.00 0.00 3 12.0 $\pm$0.4 7440 98 0.00 0.00 3 14.95$\pm$0.11 SB1
206 602 0.00 0.00 0 34.8 $\pm$0.3 7445 85 0.00 0.72 0 33.8 $\pm$1.0
240 215 0.17 0.84 3 43.3 $\pm$0.15 SB1 7488 485 0.06 0.84 0 33.0 $\pm$0.3
242 1024 0.00 0.00 3 -1.1 $\pm$0.4 7515 489 0.06 0.84 3 27.6 $\pm$0.6
277 648 0.00 0.00 3 1.6 $\pm$0.0 7551 104 0.00 0.67 3 8.9 $\pm$0.0
2086 210 0.00 0.00 0 33.3 $\pm$0.6 7663 492 0.03 0.00 3 1.5 $\pm$0.0
3128 620 0.00 0.00 3 -20.7 $\pm$0.0 7674 496 0.00 0.00 0 33.7 $\pm$0.5
4166 481 0.00 0.00 3 -2.5 $\pm$0.0 8135 566 0.00 0.78 0 34.2 $\pm$0.4
4168 482 0.00 0.00 3 39.5 $\pm$0.4 8355 623 0.00 0.63 3 49.3 $\pm$0.0
6469 453 0.00 0.00 0 34.1 $\pm$0.2 8522 657 0.00 0.00 3 12.6 $\pm$0.0
6470 468 0.00 0.70 0 33.3 $\pm$0.3 8533 632 0.00 0.76 3 67.8 $\pm$0.5
6474 495 0.00 0.73 3 9.5 $\pm$0.6 8557 250 0.00 0.00 0 33.9 $\pm$0.5
6514 261 0.00 0.00 0 34.5 $\pm$0.7 9015 744 0.10 0.81 0 33.5 $\pm$1.6
7112 37 0.00 0.00 3 -9.0 $\pm$0.0            
(*) Zero errors mean that only one measurement was taken and no dispersion could be calculated. SB1: Single-lined spectroscopic binary. SB2: Double-lined spectroscopic binary.


Source LaTeX | All tables | In the text