Tidal tails of nearby open clusters - I. Mapping with Gaia DR3

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Volume 694 (February 2025)

A&A, 694 (2025) A258

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Table A.3

Statistics of the Tidal tails we found in this work.

NAME	N_Tidal	N_Leading	N_Trailing	N_Tidal,Corr	N_Leading,Corr	N_{Trailing,Corr}	M_G,Lim	P_cont,max	a	b	r_lim
							(mag)		(km s⁻¹)	(km s⁻¹)	(pc)
ASCC 101	30	33	81	26	26	25	8.173	0.097	2.4	1.8	17
Alessi 3^*	95	91	47	75	36	32	10.114	0.090	1.6	1.0	20
Alessi 9	52	148	185	43	82	115	10.464	0.070	2.0	1.0	17
Alessi 96	65	110	60	50	66	42	8.724	0.102	3.0	1.5	20
Blanco 1	404	68	82	270	42	41	10.612	0.089	4.0	2.0	15
Collinder 350^*	53	52	130	41	42	61	7.875	0.090	2.5	1.5	23
Melotte 111^*	85	72	55	79	58	47	12.935	0.093	1.2	1.2	20
Melotte 22	1176	565	288	1144	411	272	13.17	0.098	1.5	0.9	20
Melotte 25^*	312	423	334	305	349	329	14.759	0.080	2.5	0.8	15
NGC 2632^*	973	308	147	856	168	132	11.928	0.078	2.0	1.0	17
NGC 6633	166	87	105	147	71	76	7.901	0.090	2.5	1.8	18
Platais 10^*	48	89	67	38	64	37	10.669	0.088	3.5	0.5	17
RSG 4	110	64	247	77	49	73	9.117	0.106	2.5	1.8	20
Roslund 6	191	43	123	147	34	62	8.629	0.048	1.5	1.1	17
Ruprecht 147^*	127	69	139	113	58	49	9.055	0.100	3.8	1.2	20
Stock 10^*	41	81	73	34	53	56	8.089	0.091	2.1	1.7	25
Stock 2	883	118	277	771	95	219	8.609	0.092	7.0	2.1	14
Theia 517^*	211	83	195	145	71	55	9.707	0.206	3.0	1.5	18
UPK 545	83	382	134	72	118	102	9.207	0.085	2.0	1.5	17

Column 1 : Name of the OC from HR2024,^* signifies the statistics for CP + SCCP joint sample (see Section 3.3): Columns 2 – 4 : Number of stars inside the tidal radius, the leading tail and the trailing tail ; Columns 5-7: Number of stars inside the tidal radius, the leading tail and the trailing tail for the corrected sample (see the Section 4) ; Column 8: Maximum absolute G magnitude for the correction (see Section 4); Column 9: Maximum contamination probability for k = 6 (see Section 3.1): Columns 10 – 12: Optimum neighbour finding parameters (see Section 3.2).

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