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Table 3

Probable members in open clusters and associations.

Object ASCC Pkin Pphot Cluster dist log t (μX, μY, σμ)star (μX, μY, σμ)cl
name number [%] [%] [pc] [yr] [mas/yr] [mas/yr]
HD 47839∗ 1021435 62 100 NGC 2264 660 6.81  −3.84,  −2.50, 0.94  −2.70,   −3.50,  0.25
CPD−58 2620 2232461 44 1 Trumpler 14 2753 6.67  −3.77,  −2.20, 2.37  −3.91,  3.65,  0.60
HDE 303311 2232607 91 27 Trumpler 14 2753 6.67  −2.91, 2.64, 2.40  −3.91,  3.65,  0.60
HD 93129B 2232449 0 100 Trumpler 14 2753 6.67  −9.80, 10.86, 1.96  −3.91,  3.65,  0.60
HD 93204 2232588 75 0 Trumpler 16 2842 6.90  −9.33, 3.16, 1.70  −11.10,  4.02,  0.42
HDE 303308 2232708 19 0 Trumpler 16 2842 6.90  −6.44, 2.54, 1.79  −11.10,  4.02,  0.42
HD 105056 2396832 12 100 ASCC 69 1000 7.91  −4.56,  −1.81, 0.87 7.91,   −7.52,  0.41
HD 115455 2338543 90 72 Stock 16 1640 6.78  −2.56, 1.08, 2.02  −3.31,   −0.03,  0.66
HD 120521 2256830 0 100 Platais 10 246 8.20  −5.55, 0.40, 1.39  −29.10,   −10.73,  0.40
HD 123590 2345821 83 83 ASCC 77 2200 6.99  −4.96,  −2.45, 0.99  −4.59,   −1.49,  0.47
HD 328856 2074567 22 100 Hogg 22 1297 6.70 0.78,  −1.37, 1.26  −0.84,   −4.39,  0.43
HD 135240∗ 2351294 61 100 ASCC 79 800 6.86  −3.00,  −2.65, 0.85  −2.67,   −4.10,  0.44
HD 135591∗ 2351425 67 100 ASCC 79 800 6.86  −3.00,  −2.65, 0.85  −2.67,   −4.10,  0.44
HD 152233 1974789 13 100 NGC 6231 1250 6.81  −4.11,  −8.05, 2.40  −0.39,   −1.99,  0.46
HD 152247 1974811 95 100 NGC 6231 1250 6.81  −0.55,  −1.14, 1.91  −0.39,   −1.99,  0.46
HD 152249 1974812 84 100 NGC 6231 1250 6.81 0.13,  −0.81, 1.36  −0.39,   −1.99,  0.46
HD 153919 1877055 0 100 NGC 6281 494 8.51 1.42, 4.84, 1.04  −2.96,   −3.75,  0.23
HD 154368 1877523 88 100 ASCC 88 1900 7.17 3.80,  −2.08, 1.05 2.89,   −2.00,  0.32
HD 155806 ∗ 1783567 98 100 Sco OB4 1100 6.82 0.33,  −2.02, 0.80 0.46,   −2.22,  0.15
HD 156154 1878846 82 100 Bochum 13 1077 7.08  −0.88,  −2.53, 1.64  −0.28,   −1.20,  0.30
HD 164794 ∗ 1593528 69 100 NGC 6530 1322 6.67 1.92,  −0.40, 1.09 2.01,   −1.81,  0.51
HD 315033 1593655 97 100 NGC 6530 1322 6.67 2.33,  −2.51, 2.09 2.01,   −1.81,  0.51
HD 167263∗ 1595683 97 100 Sgr OB7 1860 6.64 1.56,  −1.53, 1.19 1.80,   −1.20,  0.26
HD 168075 1407400 73 100 NGC 6611 1719 6.72 2.81,  −1.14, 1.18 1.60,   −0.35,  0.41
HD 168112 1407419 73 19 NGC 6604 1696 6.64 1.67,  −2.20, 1.69  −0.36,   −2.68,  0.31
HD 153426 1876676 0 0 Hogg 22 1297 6.70(6.91)  −0.21,  −0.09, 1.38  −0.84,   −4.39,  0.43
HD 154643 1877779 0 0 ASCC 88 1900 7.17(6.15) 3.66,  −1.71, 1.55 2.89,   −2.00,  0.32
HD 169582 1323022 0 0 NGC 6604 1696 6.64(6.74)  −0.40,  −1.63, 1.14  −0.36,   −2.68,  0.31
HD 171589 1409170 0 0 NGC 6618 1814 7.78(6.52) 5.10, 3.74, 1.66 3.04,  0.33,  0.92
HD 175754 1503597 0 0 ASCC 93 2500 7.72(7.01) 1.49, 2.15, 1.01  −2.18,   −1.80,  0.55

Notes. For each star, we give in the first two columns the object name and the corresponding catalogue number. The kinematic and photometric probabilities for cluster membership presented in Cols. 3 and 4 were calculated according to the procedures described by Kharchenko et al. (2004). The cluster names, the distances, and the ages are presented in the next three columns. The proper motions and their errors for stars and clusters are given in the last columns. All cluster data are taken from Kharchenko et al. (2005a,b). The five stars at the end of the table are currently not members of the indicated clusters, and were ejected from them tenc years ago (Schilbach & Roeser 2008). The encounter times tenc of these stars are given in brackets. The three stars with magnetic fields that are most probably cluster members are presented in italics.

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