Table A.2
Basic stellar data of the sample of UMa group members.
| Object | HIP number | α (2000.0) | δ (2000.0) | Parallax [mas] | Spec. type | V mag. | Ks mag. |
|
|
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| HD 11131 | 8486 | 01 49 23.36 | –10 42 12.8 | 44.32± 3.02 | G1V | 6.727 | 5.149 |
| HD 11171 | 8497 | 01 49 35.10 | –10 41 11.1 | 43.13± 0.26 | F3III | 4.664 | 3.872 |
| HD 22049 | 16537 | 03 32 55.84 | –09 27 29.7 | 310.94± 0.16 | K2V | 3.730 | 1.776 |
| HD 26913 | 19855 | 04 15 25.79 | +06 11 58.7 | 47.49± 0.68 | G5IV | 6.960 | 5.271 |
| HD 26923 | 19859 | 04 15 28.80 | +06 11 12.7 | 46.88± 0.47 | G0IV | 6.314 | 4.903 |
| HD 38393 | 27072 | 05 44 27.79 | –22 26 54.2 | 112.02± 0.18 | F7V | 3.586 | 2.508 |
| HD 41593 | 28954 | 06 06 40.48 | +15 32 31.6 | 65.48± 0.67 | K0V | 6.762 | 4.822 |
| HD 60491 | 36827 | 07 34 26.17 | –06 53 48.0 | 40.73± 1.00 | K2V | 8.160 | 6.019 |
| HD 61606 | 37349 | 07 39 59.33 | –03 35 51.0 | 70.37± 0.64 | K2V | 7.200 | 4.885 |
| HD 63433 | 38228 | 07 49 55.06 | +27 21 47.5 | 45.45± 0.53 | G5IV | 6.930 | 5.258 |
| HD 95650 | 53985 | 11 02 38.34 | +21 58 01.7 | 84.95± 1.05 | M0 | 9.690 | 5.688 |
| HIP 57548 | 57548 | 11 47 44.40 | +00 48 16.4 | 298.04± 2.30 | M4V | 11.080 | 5.654 |
| HD 125451 | 69989 | 14 19 16.28 | +13 00 15.5 | 38.32± 0.28 | F5IV | 5.400 | 4.394 |
| HD 135599 | 74702 | 15 15 59.17 | +00 47 46.9 | 63.11± 0.70 | K0 | 7.000 | 4.958 |
| HD 139006 | 76267 | 15 34 41.27 | +26 42 52.9 | 43.46± 0.28 | A0V+G5Va | 2.210 | 2.206 |
| HD 147584 | 80686 | 16 28 28.14 | –70 05 03.8 | 82.53± 0.52 | F9V+M4Vb | 4.910 | 3.661 |
| HD 165185 | 88694 | 18 06 23.72 | –36 01 11.2 | 56.97± 0.48 | G5V | 5.949 | 4.469 |
| HD 175742 | 92919 | 18 55 53.22 | +23 33 23.9 | 46.74± 0.85 | K0Vc | 8.090 | 5.637 |
| HIP 104383 | 104383 | 21 08 45.47 | –04 25 36.9 | 36.92± 1.53 | K6+M1d | 9.430 | 6.398 |
| HD 217813 | 113829 | 23 03 04.98 | +20 55 06.9 | 40.46± 0.57 | G5V | 6.652 | 5.148 |
Notes. All parallaxes are Hipparcos parallaxes (van Leeuwen 2007). Ks band magnitudes were taken from 2MASS (Skrutskie et al. 2006) and are combined magnitudes for tight binaries. For spectroscopic binaries, the spectral type is displayed for both components.
Reference. References for spectral type.
HD 147584: mean value of M4 of the range given by Skuljan et al. (2004) (M1V-M7V);
HD 175742: SB1 (Tokovinin et al. 2006); literature not unanimous on the parameters (Eggleton & Tokovinin 2008);
HIP 104383: Balega et al. (2004).
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