Table 2
Sample of young, nearby, and dusty stars observed during our VLT/NaCo thermal and angular differential imaging survey.
Name | α | δ | b | μαcos(δ) | μ δ | d | SpT | K | Excess? | Age | Ref. | |
HIP | HD | (J2000) | (J2000) | (deg) | (mas yr-1) | (mas yr-1) | (pc) | (mag) | (Myr) | |||
|
||||||||||||
AB Doradus | ||||||||||||
6276 | – | 01 20 32 | –11 28 03 | –72.9 | 110.69 | –138.85 | 35.06 | G9V | 6.55 | y | 70 | 1 |
⋆18 859 | 25 457 | 04 02 37 | –00 16 08 | –36.9 | 149.04 | –253.02 | 18.83 | F7V | 4.18 | y | 70 | 1 |
30 314 | 45 270 | 06 22 31 | –60 13 08 | –26.8 | –11.22 | 64.17 | 23.49 | G1V | 5.04 | y | 70 | 1 |
⋆93 580 | 177 178 | 19 03 32 | 01 49 08 | –1.86 | 23.71 | –68.65 | 55.19 | A4V | 5.32 | n | 70 | 1 |
95 347 | 181 869 | 19 23 53 | –40 36 56 | –23.09 | 32.67 | –120.81 | 52.08 | B8V | 4.20 | n | 70 | 1 |
109 268 | 209 952 | 22 08 13 | –46 57 38 | –52.47 | 127.6 | –147.91 | 31.09 | B6V | 2.02 | n | 70 | 1 |
⋆115 738 | 220 825 | 23 26 55 | 01 15 21 | –55.08 | 85.6 | –94.43 | 49.7 | A0 | 4.90 | y | 70 | 1 |
⋆117 452 | 223 352 | 23 48 55 | –28 07 48 | –76.13 | 100.03 | –104.04 | 43.99 | A0V | 4.53 | y | 70 | 1 |
|
||||||||||||
β Pictoris | ||||||||||||
⋆11 360 | 15 115 | 02 26 16 | +06 17 34 | –49.5 | 86.09 | –50.13 | 44.78 | F2 | 5.86 | y | 12 | 10 |
⋆21 547 | 29 391 | 04 37 36 | –02 28 24 | –30.7 | 43.32 | –64.23 | 29.76 | F0V | 4.54 | n | 12 | 2 |
⋆25 486 | 35 850 | 05 27 05 | –11 54 03 | –24.0 | 17.55 | –50.23 | 27.04 | F7V | 4.93 | y | 12 | 2 |
⋆27 321 | 39 060 | 05 47 17 | –51 03 59 | –30.6 | 4.65 | 83.1 | 19.4 | A6V | 3.53 | y | 12 | 2 |
⋆27 288 | 38 678 | 05 46 57 | –14 49 19 | –20.8 | 14.84 | –1.18 | 21.52 | A2IV/V | 3.29 | y | 12 | 13 |
⋆79 881 | 146 624 | 16 18 18 | –28 36 50 | +15.4 | –33.79 | –100.59 | 43.05 | A0V | 4.74 | n | 12 | 2 |
⋆88 399 | 164 249 | 18 03 03 | –51 38 03 | –14.0 | 74.02 | –86.46 | 48.14 | F5V | 5.91 | y | 12 | 2 |
⋆92 024 | 172 555 | 18 45 27 | –64 52 15 | –23.8 | 32.67 | –148.72 | 29.23 | A7V | 4.30 | y | 12 | 2 |
⋆95 261 | 181 296 | 19 22 51 | –54 25 26 | –26.2 | 25.57 | –82.71 | 48.22 | A0Vn | 5.01 | y | 12 | 2 |
⋆95 270 | 181 327 | 19 22 59 | –54 32 16 | –26.2 | 23.84 | –81.77 | 50.58 | F6V | 5.91 | y | 12 | 2 |
102 409 | 197 481 | 20 45 09 | –31 20 24 | –36.8 | 280.37 | –360.09 | 9.94 | M1V | 4.53 | y | 12 | 2 |
|
||||||||||||
Tucana-Horologium / Columba | ||||||||||||
⋆1134 | 984 | 00 14 10 | –07 11 56 | –66.36 | 102.84 | –66.51 | 46.17 | F7V | 6.07 | n | 30 | 1 |
⋆2578 | 3003 | 00 32 44 | –63 01 53 | –53.9 | 86.15 | –49.85 | 46.47 | A0V | 4.99 | y | 30 | 1 |
7805 | 10 472 | 01 40 24 | –60 59 57 | –55.1 | 61.94 | –10.56 | 67.25 | F2IV/V | 6.63 | y | 30 | 5 |
⋆9685 | 12 894 | 02 04 35 | –54 52 54 | –59.2 | 75.74 | –25.05 | 47.76 | F4V | 5.45 | n | 30 | 1 |
10 602 | 14 228 | 02 16 31 | –51 30 44 | –22.2 | 90.75 | –21.9 | 47.48 | B0V | 4.13 | n | 30 | 1 |
12 394 | 16 978 | 02 39 35 | –68 16 01 | –45.8 | 87.4 | 0.56 | 47.01 | B9 | 4.25 | n | 30 | 1 |
16 449 | 21 997 | 03 31 54 | –25 36 51 | –54.1 | 53.46 | –14.98 | 73.80 | A3IV/V | 6.10 | y | 30 | 1 |
⋆22 295 | 32 195 | 04 48 05 | –80 46 45 | –31.5 | 46.66 | 41.3 | 61.01 | F7V | 6.87 | y | 30 | 1 |
⋆26 453 | 37 484 | 05 37 40 | –28 37 35 | –27.8 | 24.29 | –4.06 | 56.79 | F3V | 6.28 | y | 30 | 1 |
26 966 | 38 206 | 05 43 22 | –18 33 27 | –23.1 | 18.45 | –13.2 6 | 69.20 | A0V | 6.92 | y | 30 | 1 |
⋆30 030 | 43 989 | 06 19 08 | –03 26 20 | –8.8 | 10.65 | –42.47 | 49.75 | F9V | 6.55 | y | 30 | 1 |
30 034 | 44 627 | 06 19 13 | –58 03 16 | –26.9 | 14.13 | 45.21 | 45.52 | K1V | 6.98 | y | 30 | 1 |
⋆107 947 | 207 575 | 21 52 10 | –62 03 08 | –44.3 | 43.57 | –91.84 | 45.09 | F6V | 6.03 | y | 30 | 1 |
⋆114 189 | 218 396 | 23 07 29 | +21 08 03 | –35.6 | 107.93 | –49.63 | 39.40 | F0V | 5.24 | y | 30 | 1 |
⋆118 121 | 224 392 | 23 57 35 | –64 17 53 | –51.8 | 78.86 | –61.1 4 | 8.71 | A1V | 4.82 | n | 30 | 1 |
|
||||||||||||
Argus | ||||||||||||
– | ⋆67 945 | 08 09 39 | –20 13 50 | +7.0 | –38.6 | 25.8 | 63.98 | F0V | 7.15 | n | 40 | 3 |
⋆57 632 | 102 647 | 11 49 04 | +14 34 19 | +70.8 | –497.68 | –114.67 | 11.00 | A3V | 1.88 | y | 40 | 3 |
|
||||||||||||
Hercules-Lyra | ||||||||||||
544 | 166 | 00 06 37 | +29 01 19 | –32.8 | 379.94 | –178.34 | 13.70 | K0V | 4.31 | y | 200 | 4 |
7576 | 10 008 | 01 37 35 | –06 45 37 | –66.9 | 170.99 | –97.73 | 23.61 | G5V | 5.70 | y | 200 | 4 |
|
||||||||||||
Upper Centaurus-Lupus | ||||||||||||
78 092 | 142 527 | 15 56 42 | –42 19 01 | –11.19 | –24.46 | 145. | F6IIIe | 4.98 | y | 5 | 6 | |
|
||||||||||||
Other | ||||||||||||
682 | 377 | 00 08 26 | +06 37 00 | +20.6 | 88.02 | –1.31 | 39.08 | G2V | 6.12 | y | 30 | 7 |
⋆7345 | 9692 | 01 34 38 | –15 40 35 | –74.8 | 94.84 | –3.14 | 59.4 | A1V | 5.46 | y | 20 | 5 |
7978 | 10 647 | 01 42 29 | –53 44 26 | –61.7 | 166.97 | –106.71 | 17.35 | F9V | 4.30 | y | 300 | 5 |
⋆13 141 | 17 848 | 02 49 01 | –62 48 24 | –49.5 | 94.53 | 29.02 | 50.68 | A2V | 5.97 | y | 100 | 5 |
18 437 | 24 966 | 03 56 29 | –38 57 44 | –49.9 | 29.46 | 0.1 | 105.82 | A0V | 6.86 | y | 10 | 5 |
22 226 | 30 447 | 04 46 50 | –26 18 09 | –37.9 | 34.34 | –4.63 | 78.125 | F3V | 6.89 | y | 100 | 5 |
⋆22 845 | 31 295 | 04 54 54 | +10 09 03 | –20.3 | 41.49 | –128.73 | 35.66 | A0V | 4.41 | y | 100 | 5 |
34 276 | 54 341 | 07 06 21 | –43 36 39 | –15.8 | 5.8 | 13.2 | 102.35 | A0V | 6.48 | y | 10 | 5 |
38 160 | 64 185 | 07 49 13 | –60 17 03 | –16.6 | –37.41 | 140.08 | 34.94 | F4V | 4.74 | n | 200 | 8 |
⋆41 307 | 71 155 | 08 25 40 | –03 54 23 | +18.9 | –66.43 | –23.41 | 37.51 | A1V | 4.08 | y | 100 | 5 |
53 524 | 95 086 | 10 57 03 | –68 40 02 | –8.1 | –41.41 | 12.47 | 90.42 | A8III | 6.79 | y | 50 | 5 |
59 315 | 105 690 | 12 10 07 | –49 10 50 | +13.1 | –149.21 | –61.81 | 37.84 | G5V | 6.05 | n | 100 | 9 |
76 736 | 138 965 | 15 40 12 | –70 13 40 | –11.9 | –40.63 | –55.31 | 78.49 | A3V | 6.27 | y | 20 | 5 |
⋆86 305 | 159 492 | 17 38 06 | –54 30 02 | –12.0 | –51.04 | –149.89 | 44.56 | A7IV | 4.78 | y | 50 | 11 |
⋆99 273 | 191 089 | 20 09 05 | –26 13 27 | –27.8 | 39.17 | –68.25 | 52.22 | F5V | 6.08 | y | 30 | 5 |
⋆101 800 | 196 544 | 20 37 49 | +11 22 40 | –17.5 | 39.15 | –8.26 | 7.94 | A1IV | 5.30 | y | 30 | 5 |
108 809 | 209 253 | 22 02 33 | –32 08 00 | –53.2 | –19.41 | 23.88 | 30.13 | F6.5V | 5.38 | y | 200 | 5 |
114 046 | 217 987 | 23 05 47 | –35 51 23 | –66.0 | 6767.26 | 1326.66 | 3.29 | M2V | 3.46 | n | 100 | 12 |
– | 219 498 | 23 16 05 | +22 10 02 | –35.6 | 79.7 | –29.4 | 150.0 | G5 | 7.38 | y | 300 | 7 |
⋆116 431 | 221 853 | 23 35 36 | +08 22 57 | –50.0 | 65.37 | –40.79 | 68.45 | F0 | 6.40 | y | 100 | 5 |
Notes. Stars with the ⋆ symbol are used for the statistical analysis. Star parameters (α, δ, b, μαcos(δ), μδ and d) are extracted from the Hipparcos catalog (van Leeuwen 2007). Unit of right ascension are hours, minutes, and seconds ; units of declination are degrees, arcminutes, and arcseconds. For HD 219498, the distance is extracted from Roccatagliata et al. (2009). The K magnitudes are extracted from the 2MASS catalog (Cutri et al. 2003). The IR excess at 24 and/or 70 μm are extracted from Zuckerman et al. (2011); Kains et al. (2011); Morales et al. (2011); Rhee et al. (2007). The age of HIP 93580 is still debated in Zuckerman et al. (2011) due to discordant kinematics. The binarity (if physical) may have some impact on both proper motions and RVs and thus on the membership to AB Dor. The age references are the following:
Reference. (1) Zuckerman et al. (2011); (2) Zuckerman et al. (2001); (3) Torres et al. (2008); (4) López-Santiago et al. (2006); (5) Rhee et al. (2007); (6) see discusion in Rameau et al. (2012); (7) Hillenbrand et al. (2008); (8) Zuckerman et al. (2006); (9) see for instance Chauvin et al. (2010); (10) Schlieder et al. (2012); (11) Song et al. (2001); (12) see discusion in Delorme et al. (2012); (13) Nakajima & Morino (2012).
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