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Table 1.

Clusters for which extratidal associations were singled out by method I.

Name α(a) δ(a) rh(b) rt(b) D(b) vr(a) μα cos δ(a) μδ(a) rμ(a) [Fe/H] (b) N< rt(c) N> rt(c)
[deg] [deg] [arcmin] [arcmin] [kpc] [km s−1] [mas yr−1] [mas yr−1] [dex]
NGC 4147 182.526 18.543 0.5 6.1 19.3 179.1 ± 0.3 −1.702 ± 0.016 −2.108 ± 0.010 −0.147 −1.80 3 19
NGC 5024 (M 53) 198.230 18.168 1.3 18.4 17.9 −63.1 ± 0.2 −0.151 ± 0.006 −1.350 ± 0.004 −0.261 −2.10 36 7
NGC 5053 199.113 17.700 2.6 11.4 17.4 42.5 ± 0.2 −0.353 ± 0.009 −1.257 ± 0.007 −0.334 −2.27 26 24
NGC 5272 (M 3) 205.548 28.377 2.3 28.7 10.2 −147.2 ± 0.2 −0.094 ± 0.004 −2.626 ± 0.003 −0.064 −1.50 181 18
NGC 6205 (M 13) 250.422 36.460 1.7 21.0 7.1 −244.4 ± 0.3 −3.172 ± 0.004 −2.586 ± 0.005 0.152 −1.53 260 32
NGC 6341 (M 92) 259.281 43.136 1.0 12.4 8.3 −120.7 ± 0.3 −4.923 ± 0.005 −0.556 ± 0.006 0.085 −2.31 75 35
NGC 7078 (M 15) 322.493 12.167 1.0 27.3 10.4 −106.5 ± 0.2 −0.622 ± 0.006 −3.782 ± 0.006 −0.037 −2.37 91 5
NGC 7089 (M 2) 323.363 −0.823 1.1 12.4 11.5 −3.6 ± 0.3 3.531 ± 0.007 −2.139 ± 0.007 0.027 −1.65 66 11

References.

(b)

Harris (1996), 2010 version.

(c)

This study.

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