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Home All issues Volume 663 (July 2022) A&A, 663 (2022) A39 Full HTML
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Table A.2.

Kinematic parameters of stellar clusters.

Name ϖ 𝜚ϖ μα* eμα* μδ eμδ RV eRV NPM NRV
Name eta Cha association 10.13 0.029 -29.83 0.4 26.99 0.29 16.69 1.11 20 2
Cl Alessi13 9.58 0.038 36.33 0.13 -4.71 0.11 21.13 3.41 48 3
Cl Platais 8 7.42 0.019 -15.6 0.09 14.47 0.08 20.64 3.41 211 32
IC 2391 6.58 0.01 -24.64 0.06 23.32 0.05 15.29 1.34 224 39
IC 2602 6.56 0.01 -17.58 0.05 10.7 0.05 17.44 1.47 311 41
Cl Melotte 20 5.67 0.007 22.86 0.05 -25.38 0.05 -0.1 2.05 764 126
NAME HIP 21974 Cluster 5.62 0.017 3.62 0.13 -20.93 0.07 8.07 1.02 90 29
NGC 2451A 5.17 0.007 -21.12 0.05 15.33 0.04 23.59 1.78 337 41
NGC 6475 3.57 0.004 3.1 0.02 -5.43 0.02 -14.63 3.33 941 164
Cl Collinder 135 3.28 0.006 -9.98 0.03 6.16 0.03 16.03 2.21 352 51
IC 348 3.08 0.013 4.48 0.05 -6.45 0.05 19.71 1.57 144 180
NAME Pozzo 1 2.85 0.005 -6.52 0.02 9.53 0.02 18.67 3.53 390 27
NGC 2547 2.55 0.005 -8.61 0.02 4.26 0.02 14.07 2.1 233 20
Cl Alessi5 2.5 0.004 -15.41 0.02 2.5 0.02 12.49 2.46 302 18
ONC 2.48 0.04 1.51 0.11 0.5 0.12 21.8 6.6 378 12
Cl Collinder 69 2.46 0.005 1.19 0.02 -2.12 0.02 29.1 3.24 669 29
Cl VDBH 164 2.36 0.006 -7.37 0.03 -10.71 0.02 -0.18 2.25 209 15
Cl Alessi20 2.31 0.007 8.2 0.03 -2.34 0.03 -11.5 0.1 124 0
Cl Trumpler 10 2.29 0.004 -12.53 0.02 6.53 0.01 22.43 2.29 478 59
Cl VDBH 99 2.23 0.004 -14.49 0.02 0.92 0.02 6.98 4.92 389 36
NGC 6405 2.17 0.004 -1.31 0.02 -5.85 0.02 -7.42 4.57 583 124
NGC 3532 2.07 0.002 -10.39 0.01 5.18 0.01 5.37 2.5 1,889 209
NGC 3532 2.07 0.002 -10.39 0.01 5.18 0.01 5.67 4.9 1,889 664
Cl Gulliver 9 1.99 0.006 -5.99 0.02 6.92 0.02 23.3 3.32 265 12
Cep OB3b 1.16 0.04 -0.75 0.09 -2.31 0.08 -28.7 4.4 678 4
Name Alessi-Teutsch 5 1.11 0.005 -1.9 0.03 -3.21 0.02 -21.04 12.12 158 2
Cl VDBH 56 1.08 0.006 -5.57 0.02 5.44 0.02 19.69 2.55 122 2
NGC 7160 1.05 0.009 -3.47 0.03 -1.38 0.03 -20.4 1.9 47 0
NGC 1502 0.92 0.005 -0.57 0.02 -0.85 0.02 -14.76 6.49 154 1
Cl Roslund 7 0.78 0.003 1.73 0.01 -0.36 0.01 -22 3 151 0
NGC 6883 0.72 0.145 -2.89 0.55 -6.53 0.6 -10.5 4.4 0 0
Cl VDBH 205 0.57 0.007 -0.15 0.02 -1.08 0.02 -2.38 19.92 96 5
Cl VDBH 211 0.52 0.009 -0.67 0.02 -1.94 0.02 -48.83 0.77 110 8
NGC 5617 0.4 0.002 -5.64 0 -3.17 0.01 -34.74 0.71 632 4
NGC 6755 0.38 0.004 -0.73 0.01 -3.53 0.01 27.11 0.88 282 8
Cl Gulliver 43 0.35 0.007 -2.92 0.02 -5.8 0.02 0.38 8.03 79 2
Teutsch 80 0.35 0.006 -5.55 0.01 -3.58 0.02 -23.48 0.43 119 2
Cl Basel 2 0.34 0.004 -4.84 0.01 -2.65 0.01 -60.07 3.47 147 5
Cl VDBH 217 0.31 0.01 -0.66 0.02 -1.83 0.01 -12.65 0.94 129 1
FSR2007 0883 0.3 0.006 0.83 0.01 -1.54 0.01 15.28 0.79 41 2
Cl Pismis 20 0.29 0.005 -3.83 0.01 -2.91 0.01 -76.71 1.01 116 1
Juchert 3 0.28 0.018 -1.51 0.04 -3.99 0.05 40.62 0.2 69 1
SAI 132 0.28 0.004 -2.38 0.01 -4.14 0.01 -32.52 2.32 175 4
Teutsch 145 0.26 0.014 -1.64 0.03 -3.44 0.03 57.92 2.67 81 1
Cl Pismis 19 0.26 0.004 -5.46 0.01 -3.25 0.01 -29.55 0.3 453 3
Kronberger 38 0.2 0.007 -5.36 0.01 2.4 0.02 -4.22 0.66 139 1

Notes. The parallaxes, the proper motions, and the radial velocities along with their respective errors are taken from literature (see text). NPM and NRV are the number of stars used for the proper motions and radial velocity calculations respectively. NRV with a value of 0 are the values taken from Conrad et al. 2017, where the number of stars is not mentioned. The clusters are shown in the descending order of their parallaxes, which explains the decrease in number of radial velocity stars for clusters farther away.

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