Kinematic parameters and membership probabilities of open clusters in the Bordeaux PM2000 catalogue

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Table 4:

The results obtained for all the extracted fields in the PM2000 zone.
Cluster	$\mu_{\alpha,c}$	$\mu_{\delta,c}$	$\mu_{\alpha,f}$	$\mu_{\delta,f}$	$\sigma_{\mu_{\alpha, f}}$	$\sigma_{\mu_{\delta, f}}$	$\rho_f$	n_c	$n_{\rm memb}$	Class
Good
NGC 2682	$-8.23\pm0.05$	$-5.72\pm0.05$	$-4.15\pm0.30$	$-5.84\pm0.25$	$7.20\pm0.22$	$6.29\pm0.20$	$-0.17\pm0.04$	$0.40\pm0.02$	502	A
Berkeley 82	$3.02\pm0.61$	$-1.64\pm0.48$	$-0.13\pm0.73$	$-2.15\pm1.24$	$1.00\pm 0.00$	$3.50\pm1.47$	$0.31\pm0.22$	$0.33\pm0.19$	16	B
NGC 1817	$2.66\pm0.18$	$-3.72\pm0.19$	$3.56\pm0.56$	$-6.70\pm0.67$	$7.16\pm0.49$	$8.59\pm0.54$	$-0.09\pm0.06$	$0.72\pm0.03$	836	B
NGC 2169	$-2.72\pm0.40$	$-4.34\pm0.41$	$-3.64\pm3.58$	$-11.46\pm4.61$	$9.30\pm2.69$	$10.75\pm3.14$	$-0.44\pm0.29$	$0.86\pm0.06$	90	B
NGC 2194	$0.07\pm0.20$	$-2.69\pm0.29$	$-0.31\pm0.26$	$-3.60\pm0.33$	$3.74\pm0.20$	$4.79\pm0.25$	$-0.08\pm0.06$	$0.21\pm0.04$	65	B
NGC 2304	$-1.78\pm0.66$	$-5.77\pm0.68$	$0.89\pm1.28$	$-2.41\pm1.51$	$3.54\pm1.23$	$4.91\pm1.31$	$-0.52\pm0.19$	$0.64\pm0.13$	78	B
NGC 2355	$-0.39\pm0.32$	$-4.78\pm0.30$	$1.03\pm0.98$	$-7.73\pm0.91$	$7.73\pm0.79$	$6.75\pm0.71$	$-0.22\pm0.10$	$0.64\pm0.06$	213	B
Intermediate
Chupina 1	$-10.54\pm0.26$	$-3.52\pm0.21$	$-3.59\pm1.02$	$-3.17\pm0.95$	$5.76\pm0.71$	$5.75\pm0.71$	$-0.09\pm0.16$	$0.30\pm0.07$	22	B
Chupina 2	$5.84\pm0.59$	$-12.50\pm0.69$	$-8.58\pm1.09$	$-6.68\pm1.19$	$3.61\pm0.73$	$3.96\pm1.05$	$-0.78\pm0.10$	$0.13\pm0.09$	3	B
Chupina 3	$-7.32\pm0.25$	$-4.37\pm0.22$	$3.18\pm2.48$	$-6.55\pm2.35$	$5.06\pm2.05$	$5.90\pm1.65$	$-0.38\pm0.32$	$0.65\pm0.12$	17	B
Chupina 4	$-9.91\pm0.37$	$-5.05\pm0.30$	$-2.06\pm1.11$	$-5.13\pm1.37$	$5.73\pm0.81$	$7.86\pm1.04$	$-0.27\pm0.15$	$0.23\pm0.08$	12	B
Chupina 5	$-8.68\pm0.35$	$-6.90\pm0.31$	$-3.12\pm1.19$	$-8.28\pm1.11$	$5.05\pm0.81$	$5.34\pm0.87$	$0.07\pm0.19$	$0.32\pm0.11$	15	B
NGC 7036	$-5.04\pm0.41$	$-6.84\pm0.35$	$0.06\pm1.26$	$-8.15\pm1.11$	$8.23\pm0.98$	$7.33\pm0.93$	$0.56\pm0.09$	$0.26\pm0.08$	20	B
Roslund 1	$-0.06\pm0.52$	$-5.09\pm0.55$	$-1.74\pm1.06$	$-7.22\pm1.17$	$7.18\pm0.89$	$8.12\pm0.99$	$-0.08\pm0.12$	$0.47\pm0.08$	70	B
Berkeley 43	$0.30\pm0.78$	$-1.81\pm0.68$	$-0.36\pm1.02$	$-3.52\pm1.65$	$4.38\pm1.02$	$8.13\pm1.31$	$0.08\pm0.16$	$0.36\pm0.15$	23	C
Berkeley 45	$-1.01\pm0.96$	$-9.27\pm0.94$	$6.28\pm1.13$	$-3.94\pm1.39$	$2.44\pm1.17$	$3.75\pm1.10$	$-0.37\pm0.33$	$0.47\pm0.12$	42	C
Berkeley 47	$0.90\pm0.90$	$-4.14\pm0.86$	$1.97\pm1.93$	$-4.93\pm2.46$	$6.79\pm1.63$	$9.65\pm2.05$	$0.65\pm0.14$	$0.60\pm0.12$	35	C
King 26	$3.80\pm0.58$	$-5.72\pm0.47$	$1.18\pm1.99$	$-6.31\pm1.73$	$7.68\pm1.72$	$6.50\pm1.58$	$0.04\pm0.22$	$0.45\pm0.15$	21	C
Skiff J0614+129	$-0.31\pm0.29$	$-2.73\pm0.37$	$-0.57\pm0.44$	$-4.31\pm0.63$	$4.48\pm0.32$	$6.56\pm0.47$	$-0.05\pm0.09$	$0.18\pm0.05$	29	C
NGC 1807	$2.06\pm0.23$	$-4.56\pm0.24$	$3.57\pm0.68$	$-7.83\pm0.75$	$7.80\pm0.57$	$8.35\pm0.59$	$-0.08\pm0.07$	$0.66\pm0.03$	529	D
NGC 2678	$-1.94\pm0.32$	$-2.00\pm0.28$	$-4.18\pm0.75$	$-5.34\pm0.57$	$8.29\pm0.55$	$6.10\pm0.43$	$-0.03\pm0.09$	$0.11\pm0.04$	16	D
Teutsch 11	$-2.24\pm0.91$	$-2.61\pm0.87$	$0.30\pm1.28$	$-4.03\pm1.41$	$5.60\pm0.97$	$6.66\pm1.13$	$0.34\pm0.17$	$0.25\pm0.14$	16	D
Poor
Berkeley 29	$0.56\pm0.45$	$-4.29\pm0.32$	$0.12\pm0.96$	$-6.46\pm0.88$	$7.43\pm0.79$	$6.26\pm0.68$	$-0.32\pm0.10$	$0.53\pm0.07$	137	B
NGC 1663	$1.13\pm0.60$	$-1.32\pm0.72$	$3.97\pm0.65$	$-4.94\pm0.72$	$6.83\pm0.51$	$7.27\pm0.55$	$-0.14\pm0.08$	$0.23\pm0.07$	49	B
NGC 2395	$1.22\pm0.38$	$-1.96\pm0.27$	$0.01\pm0.40$	$-4.32\pm0.48$	$5.80\pm0.31$	$7.17\pm0.36$	$0.01\pm0.06$	$0.27\pm0.05$	142	B
Alessi 57	$-0.92\pm0.80$	$-7.89\pm0.68$	$1.11\pm1.36$	$-4.85\pm1.94$	$5.81\pm1.22$	$9.15\pm1.55$	$-0.01\pm0.19$	$0.30\pm0.14$	14	C
Dias 8	$-4.51\pm0.48$	$-2.85\pm0.44$	$-1.13\pm1.62$	$-4.26\pm1.69$	$8.29\pm1.24$	$9.02\pm1.32$	$0.26\pm0.16$	$0.40\pm0.10$	30	C
Ivanov 2	$-1.02\pm0.73$	$0.41\pm0.89$	$-0.89\pm0.98$	$-3.62\pm1.33$	$3.29\pm0.76$	$4.56\pm0.88$	$-0.46\pm0.21$	$0.22\pm0.18$	15	C
NGC 7772	$17.50\pm0.57$	$-10.00\pm0.57$	$4.83\pm1.85$	$-8.49\pm1.63$	$7.59\pm1.33$	$6.63\pm1.21$	$0.13\pm0.23$	$0.09\pm0.06$	2	C
DolDzim 2	$1.92\pm0.49$	$-3.25\pm0.59$	$3.30\pm0.92$	$-5.57\pm1.13$	$7.23\pm0.75$	$8.79\pm0.86$	$-0.05\pm0.11$	$0.48\pm0.07$	85	D
DolDzim 7	$18.77\pm0.75$	$-12.13\pm0.70$	$-1.82\pm1.02$	$-5.70\pm1.23$	$5.79\pm0.80$	$7.56\pm0.94$	$-0.14\pm0.15$	$0.03\pm0.03$	1	D
Dolidze 26	$-0.64\pm0.18$	$-2.24\pm0.25$	$-0.96\pm0.21$	$-4.13\pm0.24$	$6.17\pm0.17$	$6.84\pm0.19$	$-0.13\pm0.03$	$0.30\pm0.02$	536	D
Dolidze 35	$3.87\pm0.36$	$0.85\pm0.37$	$0.32\pm0.78$	$-5.61\pm0.77$	$7.11\pm0.57$	$6.22\pm0.56$	$0.23\pm0.09$	$0.18\pm0.06$	28	D
Juchert 1	$-0.61\pm0.69$	$0.95\pm0.70$	$4.88\pm0.77$	$2.17\pm1.50$	$1.46\pm0.72$	$5.75\pm1.25$	$0.41\pm0.17$	$0.17\pm0.13$	4	D
Kronberger 13	$5.79\pm1.57$	$-5.39\pm1.57$	$-7.12\pm5.16$	$4.26\pm4.65$	$8.24\pm3.87$	$7.52\pm3.68$	$0.53\pm0.43$	$0.70\pm0.15$	9	D
NGC 2224	$0.66\pm0.22$	$-0.91\pm0.16$	$0.63\pm0.16$	$-3.16\pm0.20$	$4.24\pm0.13$	$5.47\pm0.15$	$-0.14\pm0.03$	$0.19\pm0.02$	252	D
NGC 2234	$0.14\pm0.07$	$-3.65\pm0.07$	$0.40\pm0.16$	$-5.88\pm0.18$	$5.48\pm0.13$	$6.11\pm0.14$	$-0.06\pm0.03$	$0.36\pm0.02$	2221	D
NGC 2265	$1.60\pm0.16$	$-2.27\pm0.19$	$1.26\pm0.31$	$-3.82\pm0.36$	$4.61\pm0.25$	$5.24\pm0.28$	$-0.12\pm0.06$	$0.31\pm0.04$	149	D
NGC 6525	$-2.39\pm0.51$	$-3.05\pm0.49$	$0.00\pm0.55$	$-2.63\pm0.75$	$5.56\pm0.45$	$8.24\pm0.61$	$0.06\pm0.08$	$0.21\pm0.06$	41	D
NGC 6738	$1.51\pm0.17$	$-2.69\pm0.17$	$-0.36\pm0.23$	$-3.93\pm0.24$	$6.44\pm0.19$	$6.71\pm0.20$	$0.22\pm0.03$	$0.18\pm0.02$	255	D
NGC 6837	$-23.18\pm2.77$	$-4.49\pm2.88$	$-0.13\pm0.66$	$-3.63\pm0.57$	$5.60\pm0.55$	$4.48\pm0.50$	$0.39\pm0.09$	$0.02\pm0.01$	5	D
NGC 6839	$0.11\pm0.66$	$-4.88\pm0.57$	$-0.05\pm0.57$	$-6.04\pm0.54$	$7.48\pm0.48$	$7.12\pm0.46$	$0.12\pm0.06$	$0.29\pm0.05$	116	D
NGC 6840	$1.08\pm0.61$	$-2.49\pm0.58$	$0.24\pm0.47$	$-6.07\pm0.51$	$6.20\pm0.41$	$6.34\pm0.40$	$0.06\pm0.06$	$0.24\pm0.06$	91	D
NGC 6843	$3.26\pm0.68$	$-1.61\pm0.66$	$0.70\pm0.51$	$-4.69\pm0.55$	$5.72\pm0.44$	$6.24\pm0.46$	$0.13\pm0.07$	$0.14\pm0.07$	33	D
NGC 6858	$-0.27\pm0.43$	$-3.35\pm0.34$	$0.46\pm0.42$	$-4.43\pm0.43$	$7.27\pm0.33$	$7.71\pm0.35$	$0.14\pm0.05$	$0.36\pm0.04$	261	D
NGC 6950	$-0.89\pm0.34$	$-6.36\pm0.39$	$-0.01\pm0.27$	$-6.38\pm0.27$	$6.44\pm0.21$	$6.72\pm0.22$	$0.42\pm0.03$	$0.09\pm0.03$	80	D
NGC 7084	$-5.50\pm0.51$	$-12.09\pm0.52$	$-0.04\pm0.47$	$-9.43\pm0.43$	$7.43\pm0.32$	$7.31\pm0.33$	$0.29\pm0.05$	$0.19\pm0.04$	97	D
Riddle 15	$2.73\pm0.90$	$-8.10\pm0.88$	$-2.42\pm3.10$	$-2.21\pm4.75$	$7.27\pm2.27$	$11.87\pm3.67$	$0.76\pm0.18$	$0.24\pm0.15$	3	D
Teutsch 12	$0.81\pm0.37$	$-1.98\pm0.35$	$-0.60\pm0.79$	$-2.89\pm0.96$	$4.97\pm0.63$	$6.22\pm0.78$	$-0.08\pm0.13$	$0.31\pm0.09$	29	D

Notes. The c subscripts indicate the parameters for the clusters, while the f subscripts indicate the fields ones. The correlation coefficient ( $\rho_f$ ), mixture proportion (n_c) and estimated number of members ( $n_{\rm memb}$ ) are adimensionals, whereas all the other parameters are in mas yr^-1 units. The ``Class'' column is the same as in Table 1. The solutions are divided following their visual classifications.

Source LaTeX | All tables | In the text

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