Table A.1
The sample of UMa group members.
| Name | Montes et al. | King et al. (2003) | Fuhrmann | Proper motion [mas/yr] | Number of | ||||
| (2001) | (2004) | ||||||||
| V pec | ρ C | kin. | phot. | final | μαcosδ | μ δ | NACO epochs | ||
|
|
|||||||||
| HD 11131 | Y | Y | ? | Y? | Y? | Y | –124.54± 3.03 | –105.82± 2.93 | 1 |
| HD 11171 | Y | Y | ?/Y? | Y? | Y? | Y | –148.11± 0.25 | –93.43± 0.24 | 2 |
| HD 22049 | ... | ... | ... | ... | ... | Y | –975.17± 0.21 | 19.49± 0.20 | 2 |
| HD 26913 | N | Y | ? | ? | ? | Y | –102.64± 0.66 | –113.30± 0.59 | 2 |
| HD 26923 | Y | Y | Y? | Y | Y? | Y | –109.46± 0.48 | –108.25± 0.43 | 1 |
| HD 38393 | Y | Y | ?/Y? | Y? | Y? | ... | –291.67± 0.14 | –368.97± 0.15 | 1 |
| HD 41593 | Y | Y | N?/? | Y | N?/? | Y | –120.46± 0.71 | –103.21± 0.43 | 2 |
| HD 60491 | N | Y | N?/? | Y? | N?/? | ... | –81.17± 1.26 | –42.66± 0.66 | 2 |
| HD 61606 | N | Y | N? | Y? | N? | ... | 69.90± 0.71 | –278.33± 0.31 | 2 |
| HD 63433 | Y | N | Y? | ? | ? | Y | –8.31± 0.65 | –10.48± 0.46 | 1 |
| HD 95650 | N | Y | Y | Y? | Y | ... | 142.30± 1.16 | –51.69± 0.79 | 1 |
| HIP 57548 | N | Y | N? | N? | N? | ... | 605.26± 2.32 | –1219.28± 1.97 | 1 |
| HD 125451 | N | Y | ... | ... | ... | ... | 105.95± 0.23 | –31.80± 0.21 | 1 |
| HD 135599 | ... | ... | ? | Y | ? | Y | 178.35± 0.66 | –137.52± 0.62 | 2 |
| HD 139006 | ... | ... | Y | Y | Y | Y | 120.27± 0.19 | –89.58± 0.20 | 2 |
| HD 147584 | ... | ... | Y | Y | Y | ... | 199.97± 0.25 | 110.97± 0.43 | 2 |
| HD 165185 | N | Y | Y | Y? | Y | ... | 105.05± 0.60 | 7.95± 0.32 | 2 |
| HD 175742 | ... | ... | N? | Y? | ? | ... | 131.31± 0.49 | –283.72± 0.63 | 2 |
| HIP 104383 | N | Y | ... | ... | ... | ... | –77.56± 2.42 | –32.89± 0.87 | 2 |
| HD 217813 | N | Y | ? | ? | ? | Y | –117.70± 0.59 | –27.66± 0.49 | 1 |
Notes. UMa membership information, proper motion (van Leeuwen 2007), and number of epochs of NACO observations obtained for the present work. We reiterate the assignments by Montes et al. (2001) and King et al. (2003) concerning the match of Eggen’s criteria or, respectively, the decision on kinematic, photometric, and final membership (“Y” = yes; “N” = no). Uncertainty is expressed by “?” and we refer the reader to King et al. (2003) for more information. Some of the stars were not observed (zero NACO epochs taken) as is explained in the text and omitted here.
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