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Table 2:

Global properties of the remaining 29 clusters of the WINGS sample.
Cluster RA Dec z Nz $\sigma_L$ Refs. log (LX)
  (J2000) (J2000)     km s-1   1044 erg s-1
A0085 00:41:37.81 -09:20:33.2 0.0521 273 979 ag07 44.92
A0133 01:02:38.97 -21:57:15.4 0.0603 7 623 st99 44.55
A0147 01:08:10.44 +02:09:59.9 0.0447 11 387 st99 43.73
A0168 01:15:09.80 +00:14:50.6 0.0448 106 578 ag07 44.04
A0311 02:09:10.34 +19:43:10.4 0.0657 1 ... wu98 43.91
A0548b 05:47:01.74 -25:36:58.8 0.0441 323 842 st99 43.48
A0602 07:53:19.02 +29:21:10.5 0.0621 78 834 ag07 44.05
A0780 09:18:30.36 -12:15:40.1 0.0565 34 $\ldots$ FPS04 44.82
A1668 13:03:51.41 +19:15:55.1 0.0634 15 654 st99 44.20
A1736 13:26:52.16 -27:06:33.5 0.0461 109 918 st99 44.37
A2149 16:01:38.10 +53:52:42.9 0.0675 20 459 ag07 43.92
A2256 17:03:43.53 +78:43:02.6 0.0581 116 1376 st99 44.85
A2271 17:17:17.53 +78:01:00.0 0.0584 10 460 st99 43.80
A2657 23:44:51.00 +09:08:39.6 0.0400 31 829 st99 44.20
A2665 23:50:45.44 +06:06:41.2 0.0562 2 $\ldots$ st99 44.28
A2717 00:02:59.40 -36:02:05.5 0.0498 56 512 st99 44.00
A2734 00:11:20.13 -28:52:18.5 0.0624 80 628 st99 44.41
A3164 03:45:49.70 -57:02:43.9 0.0611 3 991 st99 44.17
A3528a 12:54:31.28 -29:22:21.6 0.0535 28 969 maz96 44.12
A3528b 12:54:08.64 -28:50:32.5 0.0535 6 $\ldots$ FPS04 44.30
A3530 12:55:36.88 -30:21:14.4 0.0544 $\ldots$ 391 wu98 43.94
A3532 12:57:19.17 -30:22:12.7 0.0555 44 742 st99 44.45
A3558 13:27:54.77 -31:29:31.8 0.0477 341 977 st99 44.80
A3562 13:33:31.81 -31:40:22.5 0.0502 114 1048 st99 44.52
A3667 20:12:30.09 -56:48:59.5 0.0530 162 1059 st99 44.94
A3716 20:51:16.71 -52:41:43.5 0.0448 111 733 st99 44.00
A3880 22:27:49.53 -30:34:40.0 0.0570 22 855 st99 44.27
A4059 23:56:40.70 -34:40:17.7 0.0480 45 628 FPS04 44.49
Z1261 07:16:42.60 +53:24:28.0 0.0644 $\ldots$ $\ldots$ wu98 43.91
Refs: (st94) Struble & Ftaclas (1994); (g96) Girardi et al. (1996); (maz96) Mazure et al. (1996); (wu98) Wu et al. (1998); (st99) Struble & Rood (1999); (FPS04) Smith et al. (2004); (ag07) Aguerri et al. (2007).
Columns: (1) cluster name, (2-3) coordinates of the image field center at epoch 2000 (right ascension (2) in hours, minutes and seconds and declination (3) in degrees, arcminutes, arcseconds), (4) cluster mean redshift, (5) number of member galaxies, (6) cluster velocity dispersion (7) reference for the data reported in columns (4-6), (8) logarithm of the X-ray luminosity in the 0.1-2.4 keV ROSAT RASS bandpass (from Ebeling et al. 1996).

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