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Home All issues Volume 497 / No 1 (April I 2009) A&A, 497 1 (2009) 209-242 Full HTML
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Table 2:

Data from Nicolet (1981) for the cluster NGC 752.
Id HD HIP $\varpi$ (mas) $\Delta m$
88 160 915 86 736 $56.65\pm0.24$ 6.834
123 109 085 61 174 $54.70\pm0.17$ 6.815
139 139 664 76 829 $57.35\pm0.16$ 6.957
235 7439 5799 $42.76\pm0.30$ 6.165
259 22 001 16 245 $46.12\pm0.13$ 6.565
266 22 001 16 245 $46.12\pm0.13$ 6.430
273 43 318 29716 $26.89\pm0.31$ 5.727
273 201 772 104 738 $30.34\pm0.34$ 5.987
304 70 958 41 211 $37.57\pm0.33$ 6.188
401 4813 3909 $63.48\pm0.35$ 6.876
402 189 245 98 470 $47.06\pm0.41$ 6.295
401 191 862 99 572 $36.10\pm0.41$ 6.079
401 196 378 101 983 $40.55\pm0.27$ 7.032
402 40 136 28 103 $67.21\pm0.25$ 7.144
403 193 307 100 412 $32.24\pm0.47$ 6.144
403 221 356 116 106 $38.29\pm0.54$ 5.820
414 198 188 102 762 $17.11\pm0.88$ 4.759
416 88 742 50 075 $43.77\pm0.41$ 6.459
416 210 918 109 821 $37.57\pm0.33$ 6.186
428 104 731 58 803 $39.49\pm0.28$ 6.420
430 221 356 116 106 $38.29\pm0.54$ 5.905
432 23 754 17 651 $56.73\pm0.19$ 7.115
The identifier in Col. 1 comes from a proper motion study of this cluster by Ebbighausen (1939). The identifiers in Cols. 2 and 3 apply to the comparison star. Column 4 gives the parallaxes from the new Hipparcos reduction.

Source LaTeX | All tables | In the text

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