Clusters of Galaxies in a Weyl Geometric Approach to Gravity
Table 1
Properties of the 19 galaxy clusters (Table of [2]).
Name
X-ray center (J2000)
Redshift
Undisturbed/cool-core
RA
Dec
A0085
00:41:50.306
−09:18:11.11
0.0556
6.37 ± 1.00
5.68 ± 0.37
8.13 ± 0.38
7.36 ± 1.00
Y/S
A0400
02:57:41.349
+06:01:36.93
0.0240
1.83 ± 0.39
1.07 ± 0.07
1.36 ± 0.05
4.39 ± 1.06
N/N
IIIZw54
03:41:18.729
+15:24:13.91
0.0311
1.91 ± 0.58
1.18 ± 0.08
1.45 ± 0.26
4.57 ± 0.56
Y/W
A1367
11:44:44.501
+19:43:55.82
0.0216
1.76 ± 0.27
2.11 ± 0.14
2.07 ± 0.07
4.35 ± 0.74
N/N
MKW4
12:04:27.660
+01:53:41.50
0.0200
0.50 ± 0.14
0.58 ± 0.04
0.47 ± 0.02
1.16 ± 0.22
Y/S
ZwCl1215
12:17:40.637
+03:39:29.66
0.0750
4.93 ± 0.98
4.34 ± 0.28
6.10 ± 0.29
7.05 ± 0.83
Y/N
A1650
12:58:41.885
−01:45:32.91
0.0845
3.44 ± 0.66
4.28 ± 0.27
5.09 ± 0.73
7.47 ± 1.13
Y/W
Coma
12:59:45.341
+27:57:05.63
0.0232
6.55 ± 0.79
6.21 ± 0.40
8.42 ± 0.63
13.14 ± 1.80
N/N
A1795
13:48:52.790
+26:35:34.36
0.0616
3.41 ± 0.63
4.46 ± 0.29
5.11 ± 0.14
6.21 ± 0.98
Y/S
MKW8
14:40:42.150
+03:28:17.87
0.0270
0.62 ± 0.12
1.10 ± 0.07
0.80 ± 0.12
1.61 ± 0.23
N/N
A2029
15:10:55.990
+05:44:33.64
0.0767
14.70 ± 2.61
6.82 ± 0.44
13.35 ± 0.53
9.59 ± 1.11
Y/S
A2052
15:16:44.411
+07:01:12.57
0.0348
1.39 ± 0.28
2.03 ± 0.13
1.86 ± 0.10
3.53 ± 0.40
Y/S
MKW3S
15:21:50.277
+07:42:11.77
0.0450
1.45 ± 0.34
2.29 ± 0.15
2.13 ± 0.09
3.90 ± 0.43
Y/S
A2065
15:22:29.082
+27:43:14.39
0.0721
11.18 ± 1.78
3.35 ± 0.22
7.66 ± 1.44
7.32 ± 0.75
N/W
A2142
15:58:19.776
+27:14:00.96
0.0899
7.36 ± 1.25
10.26 ± 0.66
13.76 ± 0.73
8.42 ± 0.77
Y/W
A2147
16:02:16.305
+15:58:18.46
0.0351
4.44 ± 0.67
3.63 ± 0.23
5.04 ± 0.53
6.84 ± 0.90
N/N
A2199
16:28:37.126
+39:32:53.29
0.0302
2.69 ± 0.42
2.64 ± 0.17
2.97 ± 0.30
4.76 ± 0.50
Y/S
A2255
17:12:54.538
+64:03:51.46
0.0800
7.13 ± 1.38
4.08 ± 0.26
7.11 ± 0.33
6.74 ± 0.97
N/N
A2589
23:23:56.772
+16:46:33.19
0.0416
3.03 ± 0.75
1.88 ± 0.12
2.54 ± 0.17
5.12 ± 0.56
Y/W
Notes. The cluster mass, , is derived from the relation and only used for comparison with the cluster mass, , derived from the “harmonic” velocity dispersion. “S,” “W,” and “N” denote strong cool-core, weak cool-core, and noncool-core clusters.
