Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution

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Volume 615 (July 2018)

A&A, 615 (2018) A49

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Table 3

Selected parameters for 36 integrated orbits.

OC	Log age	U_S	V_S	W_S	z	z_max	e
					[pc]	[pc]
IC 4725	7.97	13.7 ± 0.5	−4.4 ± 1.4	10.4 ± 1.1	−25 ± 9	92 ± 9	0.086 ± 0.021
IC 4756	9.09	−15.3 ± 0.3	−3.4 ± 0.3	2.3 ± 0.3	72 ± 5	72 ± 5	0.087 ± 0.004
NGC 0752	9.17	−13.1 ± 0.3	−6.0 ± 0.5	−9.5 ± 0.3	−141 ± 14	229 ± 30	0.069 ± 0.009
NGC 1342	8.6	11.9 ± 0.4	8.5 ± 0.6	8.1 ± 0.5	−170 ± 19	196 ± 17	0.035 ± 0.003
NGC 1647	8.3	18.8 ± 0.3	14.0 ± 0.3	6.5 ± 0.3	−125 ± 11	148 ± 8	0.06 ± 0.0
NGC 1662	9.03	26.1 ± 0.4	15.5 ± 0.2	10.2 ± 0.3	−121 ± 10	177 ± 7	0.084 ± 0.001
NGC 2099	8.95	−1.1 ± 0.3	−30.6 ± 4.0	1.2 ± 1.8	81 ± 13	93 ± 24	0.138 ± 0.042
NGC 2168	8.26	23.1 ± 0.3	0.1 ± 0.6	2.8 ± 0.5	59 ± 7	64 ± 5	0.081 ± 0.01
NGC 2281	8.85	−15.1 ± 0.2	4.8 ± 0.5	−3.1 ± 0.6	176 ± 18	188 ± 25	0.059 ± 0.006
NGC 2360	8.8	−4.8 ± 1.1	17.9 ± 1.1	24.6 ± 1.2	−9 ± 8	415 ± 120	0.055 ± 0.027
NGC 2423	9.03	26.4 ± 0.5	−7.9 ± 0.5	−0.8 ± 0.6	88 ± 10	104 ± 20	0.12 ± 0.013
NGC 2447	8.68	−1.4 ± 0.8	10.8 ± 0.6	5.6 ± 0.6	27 ± 0	68 ± 9	0.023 ± 0.01
NGC 2477	8.91	35.7 ± 4.4	10.7 ± 2.4	9.6 ± 5.2	−115 ± 49	198 ± 59	0.098 ± 0.032
NGC 2527	9.03	−15.1 ± 0.3	−8.6 ± 0.2	6.8 ± 0.2	42 ± 1	97 ± 1	0.107 ± 0.004
NGC 2539	8.96	8.3 ± 1.0	−9.3 ± 0.9	2.5 ± 1.7	196 ± 54	211 ± 62	0.106 ± 0.009
NGC 2546	8.13	4.2 ± 1.3	10.9 ± 0.8	−1.9 ± 0.8	−13 ± 9	27 ± 12	0.022 ± 0.005
NGC 2548	8.9	14.4 ± 0.6	15.8 ± 0.6	14.2 ± 0.7	211 ± 27	297 ± 27	0.05 ± 0.005
NGC 2567	8.87	10.4 ± 1.7	−5.5 ± 1.0	−2.3 ± 1.2	123 ± 48	156 ± 68	0.097 ± 0.016
NGC 2682	9.54	−19.0 ± 1.7	−11.0 ± 1.3	−3.0 ± 2.9	392 ± 80	403 ± 93	0.111 ± 0.006
NGC 3680	9.2	−1.8 ± 2.5	1.8 ± 0.7	−0.3 ± 1.0	264 ± 34	266 ± 33	0.036 ± 0.003
NGC 5138	7.55	0.4 ± 6.5	−7.8 ± 3.5	5.2 ± 1.6	98 ± 21	108 ± 27	0.06 ± 0.021
NGC 5316	8.23	−39.5 ± 5.0	−26.0 ± 3.1	21.2 ± 0.9	27 ± 0	84 ± 3	0.05 ± 0.028
NGC 5617	8.25	−62.5 ± 20.4	−35.2 ± 11.1	22.8 ± 2.9	21 ± 1	64 ± 30	0.073 ± 0.029
NGC 5662	8.28	−22.0 ± 1.0	−3.1 ± 0.9	0.9 ± 0.4	69 ± 5	128 ± 19	0.04 ± 0.008
NGC 5822	9.15	−31.0 ± 0.8	−6.2 ± 0.8	13.5 ± 0.4	78 ± 10	81 ± 9	0.066 ± 0.01
NGC 6067	7.97	−0.7 ± 4.5	−7.6 ± 4.9	14.4 ± 2.5	−88 ± 77	117 ± 61	0.1 ± 0.071
NGC 6124	8.29	−3.5 ± 0.4	20.3 ± 0.7	7.0 ± 0.7	88 ± 7	107 ± 6	0.037 ± 0.002
NGC 6134	9.02	−2.8 ± 1.1	17.8 ± 2.1	−8.3 ± 2.6	21 ± 0	99 ± 50	0.025 ± 0.007
NGC 6281	8.8	6.9 ± 0.4	6.2 ± 0.9	9.7 ± 0.9	47 ± 2	89 ± 8	0.038 ± 0.005
NGC 6494	8.52	−2.4 ± 0.2	16.7 ± 0.9	4.5 ± 1.0	71 ± 7	76 ± 3	0.019 ± 0.005
NGC 6705	8.51	35.5 ± 4.7	−4.2 ± 7.0	4.4 ± 4.0	−45 ± 50	102 ± 70	0.157 ± 0.039
NGC 6811	8.8	28.3 ± 3.5	16.4 ± 0.5	22.1 ± 1.4	206 ± 38	281 ± 47	0.077 ± 0.004
NGC 6866	8.64	7.7 ± 4.6	27.1 ± 0.6	8.8 ± 3.8	175 ± 46	212 ± 57	0.078 ± 0.001
NGC 6940	8.98	24.8 ± 1.6	9.5 ± 0.5	−10.5 ± 0.9	−99 ± 13	205 ± 36	0.075 ± 0.005
NGC 7209	9.01	−22.4 ± 1.2	−5.4 ± 0.4	5.1 ± 0.9	−81 ± 23	114 ± 11	0.09 ± 0.013
Trumpler 3	8.01	18.2 ± 1.6	31.2 ± 1.8	−8.0 ± 1.1	78 ± 9	84 ± 12	0.054 ± 0.005

Notes. The velocity U_S is positive towards the Galactic centre, V_S along the Galactic rotation, and W_S towards the Galactic north pole. The uncertainties were derived from 10 000 random realisations, varying the cluster distance, proper motion, and radial velocity according to their uncertainties.

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