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Table A.1

Stellar parameters.

Star V B−V Method vsini Teff
[km s-1] [K]
BD 182366A 9.370 0.83 −4.56 U 2.0 5308
BD 182366B 9.427 0.93 −4.57 U 2.4 5290
BD 222706A 9.594 0.62 −4.97 D 2.3 5943
BD 222706B 9.828 0.69 −4.51 U 2.3 5674
BD 231978A 9.395 0.83 −4.46 D 3.5 4886
BD 231978B 9.530 0.75 −4.44 U 3.2 4911
HD 105421A 7.827 0.51 −4.70 U 4.6 6324
HD 105421B 8.358 0.57 −4.65 U 0.9 6102
HD 106515A 7.960 0.79 −5.04 D 1.7 5314
HD 106515B 8.234 0.83 −5.07 D 1.8 5157
HD 108421A 8.870 0.90 −4.57 X 2.6 4700
HD 108421B 9.274 0.88 −4.53 X 3.2 4779
HD 108574 7.418 0.56 −4.49 D 4.9 6205
HD 108575 7.972 0.67 −4.43 X 5.1 5895
HD 109628A 9.073 0.57 −4.51 U 3.0 6109
HD 109628B 9.087 0.55 −4.50 U 3.2 6127
HD 117963A 8.639 0.55 −4.65 U 6.2 6180
HD 117963B 8.924 0.49 −4.61 U 3.3 6097
HD 118328A 9.147 0.62 −4.61 U 0.7 5943
HD 118328B 9.426 0.69 −4.59 U 0.7 5887
HD 121298A 8.604 0.50 −4.91 D 1.9 6353
HD 121298B 8.937 0.52 −4.87 D 1.3 6266
HD 123963A 8.758 0.62 −4.63 U 1.6 5873
HD 123963B 9.511 0.60 −4.55 U 1.4 5438
HD 124054A 8.399 0.58 −4.97 D 2.7 6081
HD 124054B 8.785 0.64 −5.02 D 2.5 5896
HD 126246A 7.466 0.54 −4.40 D 7.9 6223
HD 126246B 7.697 0.60 −4.51 D 3.9 6074
HD 128041A 8.059 0.71 −4.53 U 3.4 5663
HD 128041B 8.827 0.78 −4.51 U 3.2 5192
HD 132563A 8.948 0.54 −4.62 U 3.9 6168
HD 132563B 9.402 0.57 −4.62 U 3.4 5985
HD 132844A 9.022 0.55 −4.66 U 3.4 5878
HD 132844B 9.114 0.63 −4.61 U 2.4 5809
HD 13357A 8.180 0.67 −4.70 D 1.7 5615
HD 13357B 8.647 0.73 −4.61 D 1.8 5341
HD 135101A 6.656 0.69 −4.99 D 2.3 5631
HD 135101B 7.500 0.75 −5.07 D 1.1 5491
HD 139569A 8.482 0.54 −4.55 U 8.5 6223
HD 139569B 8.783 0.57 −4.52 U 5.6 5922
HD 143144A 8.856 0.62 −4.61 U 1.9 5943
HD 143144B 9.025 0.61 −4.59 U 1.2 5894
HD 146413A 9.260 0.88 −4.68 D 2.1 4779
HD 146413B 9.492 0.87 −4.60 X 2.0 4818
HD 17159A 8.775 0.54 −4.64 U 3.4 6155
HD 17159B 8.923 0.53 −4.62 U 2.9 6051
HD 186858A 8.368 0.96 −4.73 D 3.6 4910
HD 186858B 8.578 0.93 −4.62 X 3.0 4885
HD 190042A 8.755 0.73 −4.71 U 3.5 5474
HD 190042B 8.778 0.80 −4.72 U 3.8 5406
HD 19440A 7.874 0.47 −4.73 U 4.5 6308
HD 19440B 8.574 0.53 −4.66 U 2.9 6108
HD 200466A 8.399 0.74 −4.77 D 2.0 5633
HD 200466B 8.528 0.76 −4.69 D 2.1 5583
HD 201936A 8.648 0.48 −4.55 X 8.8 6441
HD 201936B 8.851 0.50 −4.53 X 15.5 6452
HD 209965A 7.980 0.55 −4.96 D 4.2 6180
HD 209965B 8.414 0.57 −4.59 U 2.1 6115
HD 213013A 8.982 0.81 −4.59 U 1.7 5402
HD 213013B 9.612 0.93 −4.53 U 2.3 4990
HD 215812A 7.275 0.64 −4.66 U 1.3 5688
HD 215812B 7.576 0.71 −4.64 U 1.5 5586
HD 216122A 8.062 0.58 −4.73 U 6.5 6067
HD 216122B 8.186 0.58 −4.71 U 4.6 6066
HD 219542A 8.174 0.64 −5.07 D 2.1 5849
HD 219542B 8.547 0.72 −4.81 D 1.9 5691
HD 2770A 9.566 0.61 −4.39 X 2.8 5970
HD 2770B 9.660 0.73 −4.39 X 3.9 5844
HD 30101A 8.782 0.82 −4.72 D 1.9 5143
HD 30101B 8.848 0.91 −4.79 D 2.2 5061
HD 33334A 8.023 0.70 −4.99 D 1.9 5650
HD 33334B 8.857 0.80 −4.63 U 1.7 5201
HD 66491A 9.253 0.75 −4.65 D 2.5 5497
HD 66491B 9.312 0.67 −4.58 D 2.4 5492
HD 76037A 7.688 0.50 −5.14 D 7.9 6353
HD 76037B 8.269 0.50 −5.03 D 9.5 6442
HD 8009A 8.819 0.64 −4.96 D 0.2 5688
HD 8009B 9.724 0.82 −4.95 D 0.0 5291
HD 8071A 7.312 0.57 −4.74 U 5.5 6218
HD 8071B 7.573 0.60 −4.71 U 6.0 6142
HD 85441A 8.907 0.70 −4.60 X 1.3 5701
HD 85441B 9.284 0.71 −4.56 X 1.6 5537
HD 86057A 8.839 0.60 −4.49 X 6.0 6012
HD 86057B 9.676 0.73 −4.40 X 4.6 5629
HD 87743A 8.734 0.62 −4.71 D 2.5 5943
HD 87743B 8.890 0.60 −4.59 D 3.0 5905
HD 94399A 9.407 0.61 −4.54 X 3.2 5970
HD 94399B 9.306 0.71 −4.56 X 3.6 6017
HD 9911A 9.428 0.90 −4.60 U 1.3 5000
HD 9911B 9.448 0.89 −4.60 U 1.3 4968
HD 99121A 8.162 0.46 −4.67 U 6.7 6501
HD 99121B 9.018 0.47 −4.57 U 5.0 6374
HIP 104687A 8.144 0.64 −4.41 D 3.0 5870
HIP 104687B 8.189 0.71 −4.48 D 3.4 5801
14 Her 6.610 0.88 −5.06 D 1.6 5388
40 Eri 4.430 0.65 −4.90 D 0.5 5151
51 Peg 5.450 0.67 −5.08 D 2.0 5787
61 Cyg B 6.030 1.31 −4.95 D 1.7 4077
83 LeoA 6.490 1.00 −4.84 D 1.4 5502
GJ 380 6.610 1.33 −4.72 D 1.9 3876
GJ 580A 6.580 0.78 −5.11 D 2.1 5174
HD 166435 6.840 0.58 −4.27 D 7.6 5964
ρ CrB 5.390 0.61 −5.08 D 1.0 5823
τ Cet 3.490 0.73 −4.98 D 1.0 5283

Notes. For each star we indicate the apparent V magnitude, the B−V color index, the method used to calculate and its value, the projected velocity vsini and temperature. values were derived from direct measurement (D) of other authors, from the X-ray luminosity (X), or can be only an upper limits (U), still from X-ray luminosity data.

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