Table 2.
Comparison between the pseudo-photometric and TGAS distances for 11 additional clusters.
Name | α (degr) | μα | μδ | ppdm1 | ppdm2 | tgdm (this work) |
---|---|---|---|---|---|---|
ClustID | δ (degr) | σμα | σμδ | NStar | NStar | NStar |
Stock 2 | 34.00 | 15.38 | −13.49 | 7.61 ± 0.02 | 7.59 ± 0.03 | 7.69 ± 0.08 |
C0211+590 | 59.50 | 0.19 | 0.11 | 51 | 34 | 64 |
Collinder 70 | 83.57 | 0.15 | −0.66 | 8.05 ± 0.02 | 8.02 ± 0.04 | 7.95 ± 0.08 |
C0533−011 | −1.27 | 0.18 | 0.11 | 66 | 33 | 130 |
NGC 1647 | 71.51 | −2.28 | −2.92 | 8.65 ± 0.02 | 8.65 ± 0.02 | 8.59± 0.09 |
C0443+189 | 19.08 | 0.36 | 0.42 | 66 | 45 | 40 |
NGC 2264N | 100.33 | −2.49 | −4.66 | 7.53 ±0.03 | 7.49 ± 0.09 | – |
C0638+099 | 9.82 | 0.44 | 0.90 | 66 | 18 | |
NGC 2264F | 100.26 | −2.37 | −4.15 | 9.19 ±0.04 | 9.17 ± 0.07 | 9.26 ± 0.15 |
C0638+099 | 9.80 | 0.43 | 0.40 | 30 | 11 | 14 |
NGC 7243 | 333.84 | −1.94 | −2.54 | 9.43 ± 0.04 | 9.42 ± 0.03 | 9.30 ± 0.10 |
C2213+496 | 49.84 | 0.36 | 0.20 | 49 | 19 | 70 |
M 67 | 132.84 | −8.13 | −5.78 | 9.44 ± 0.02 | 9.40 ± 0.02 | 9.26 ± 0.20 |
C0847+120 | 11.80 | 0.11 | 0.12 | 167 | 123 | 23 |
NGC 6811 | 294.32 | −4.92 | −8.24 | 9.51 ± 0.06 | – | 9.51 ± 0.18 |
C1936+464 | 46.38 | 0.15 | 0.10 | 35 | 12 | |
M 29 | 305.79 | −2.89 | −2.78 | 11.10 ± 0.02 | – | 11.24 ± 0.17 |
C2022+383 | 38.61 | 0.31 | 0.43 | 98 | 48 | |
NGC 869 | 34.76 | −1.02 | −0.99 | 11.53 ± 0.03 | – | 11.42 ± 0.21 |
C0215+569 | 57.14 | 0.11 | 0.04 | 135 | 38 | |
NGC 884 | 35.52 | −0.99 | −1.02 | 11.66 ± 0.04 | – | 11.60 ± 0.19 |
C0218+568 | 57.14 | 0.13 | 0.07 | 77 | 66 | |
Trumpler 16 | 161.22 | −7.29 | 2.93 | 11.80 ± 0.02 | – | 11.88 ± 0.47 |
C1043−594 | −59.68 | 0.14 | 0.16 | 16 | 10 |
Notes. Col. 1: cluster name; Col. 2: position RA (J2000), Dec (J2000); Col. 3: RA proper motion and error (mas yr−1); Col. 4: Dec proper motion and error (mas yr−1); Col. 5: ppdm1, pseudo-photometric distance without proper motion constraint; Col. 6: ppdm2, pseudo-photometric distance with proper motion constraint; Col. 7: TGAS distance from this paper.
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