Table A.2
TGAS stars with HSOY proper motions in the V1062 Sco moving group.
No. | Name | RA (J2000) | Dec (J2000) | μα | μδ | ϖkin | ϖTGAS | J | H | KS | G | Membership | H | X |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(deg) | (deg) | (mas yr−1) | (mas yr−1) | (mas) | (mas) | (mag) | (mag) | (mag) | (mag) | |||||
51 | HD 149638 | 249.429970 | −39.708627 | −13.21 | −20.97 | 5.69 ± 0.23 | 5.71 ± 0.22 | 8.862 | 8.539 | 8.425 | 10.097 | m(5d) | H | – |
52 | HD 150165 | 250.234747 | −40.187218 | −11.27 | −22.49 | 5.77 ± 0.15 | 5.83 ± 0.28 | 8.304 | 8.049 | 7.950 | 9.280 | nm (kin) | H | – |
53 | HD 149738 | 249.612316 | −39.651811 | −11.73 | −20.80 | 5.48 ± 0.06 | 6.07 ± 0.32 | 7.683 | 7.658 | 7.607 | 7.955 | m(5d) | H | – |
54 | HD 322024 | 251.071987 | −40.252976 | −14.11 | −20.20 | 5.63 ± 0.25 | 0.71 ± 0.87 | 6.533 | 5.687 | 5.410 | 8.967 | nm (kin) | – | – |
55 | HD 149336 | 248.895070 | -37.110095 | −11.44 | −22.61 | 5.80 ± 0.15 | 6.17 ± 0.25 | 8.486 | 8.249 | 8.237 | 9.399 | nm (RV) | H | – |
56 | HD 149984 | 249.946029 | −38.769026 | −13.02 | −21.86 | 5.83 ± 0.22 | 5.79 ± 0.22 | 9.232 | 8.951 | 8.872 | 10.051 | m(6d) | H | – |
57 | HD 321981 | 251.376202 | −39.161844 | −11.63 | −21.44 | 5.59 ± 0.24 | 5.00 ± 0.38 | 9.300 | 8.787 | 8.690 | 10.741 | m(5d) | – | X |
58 | HD 151868 | 252.940040 | −38.052476 | −12.32 | −21.31 | 5.63 ± 0.18 | 5.90 ± 0.22 | 8.593 | 8.427 | 8.345 | 9.281 | m(5d) | – | – |
59 | HD 152369 | 253.642044 | −38.105640 | −12.05 | −22.56 | 5.85 ± 0.09 | 6.24 ± 0.92 | 8.262 | 8.204 | 8.159 | 8.710 | m(5d) | H | – |
Notes. The columns of the table are listed as follows: Col. 1 lists the internal star number in the V1062Sco MG and Col. 2 lists the main identifier of the star in SIMBAD; Cols. 3 and 4 give the right ascension and declination, and Cols. 5 and 6 give the proper motions in right ascension and declination in the HSOY catalogue; Col. 7 lists the kinematic parallax and its mean error from the CP method,and Col. 8 gives the trigonometric parallax and its mean error from TGAS; Cols. 9 to 11 list the J, H, KS magnitudes from 2MASS; Col. 12 gives the mean G magnitude from Gaia DR1, Col. 13 gives the membership information (and comments), and Cols. 14 and 15 list the crossmatch with Hoogerwerf (2000) and ROSAT-2RXS (Boller et al. 2016).
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