The distribution of lenticular galaxies in the phase space of present-day galaxy cluster regions

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Volume 697 (May 2025)

A&A, 697 (2025) A163

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Table 2.

Main properties of MR clusters.

ID	Abell # ^(a)	N_tot^(b)	N_clu	z_clu	RA[deg]	Dec[deg]	R_vir[Mpc]	M_vir[ $10^{14} M_{⊙}$ $10^{14} \,\text{ M}_{\odot}$ ]	σ_clu[km s⁻¹]
205	A1691	205	89	0.073	197.8042	39.2410	2.7500	12.1095	877.61
262	A1809	195	90	0.080	208.2826	5.1494	2.3297	7.3625	751.00
292	A1904	239	107	0.072	215.5512	48.5482	2.5564	9.7271	814.73
571	A1663	219	83	0.084	195.6563	−2.4993	2.5500	9.6545	826.23
734	A2028	153	65	0.077	227.3734	7.5756	2.2285	6.4442	715.59
804	−	55	33	0.073	232.3093	52.8827	1.5800	2.2966	504.66
2236	−	100	42	0.063	208.0137	46.3524	1.7392	3.0631	547.36
2316	−	70	39	0.072	163.5068	54.8142	1.6252	2.4992	518.04
2496	A1913	163	83	0.054	216.6968	16.6641	1.6612	2.6690	516.35
2620	−	160	62	0.039	233.1474	4.6955	1.6657	2.6908	506.75
5183	A1377	125	74	0.052	176.8621	55.7434	2.3043	7.1240	713.87
5567	−	175	90	0.045	230.4534	7.6990	2.0760	5.2096	636.96
5905	A1185	204	126	0.032	167.7492	28.6817	1.8806	3.8722	566.50
8062	A1314	197	115	0.033	173.7296	49.0778	2.5326	9.4584	764.11

Mean ^(c)	−	161	78	0.061	−	−	2.1057	6.0129	661.42

Notes.

^(a)

Cluster number in the Abell catalog.

^(b)

Total number of galaxies in the cluster region. Descriptions of the variables in the remaining columns are provided in the text.

^(c)

Mean of the values in the columns, when applicable.

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