Internal kinematics of spiral galaxies in distant clusters - IV. Gas kinematics of spiral galaxies in intermediate redshift clusters and in the field

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Table 1:

Basic galaxy cluster information.
Name	z	Ref.	$R_{\rm vir}$	Ref.	$\sigma$	Ref.	$L_{\rm X}$	Ref.	Dynamical state	Ref.	N
			$(h^{-1}~{\rm Mpc})$		$\rm km~s^{-1}$		$(10^{44}~{\rm erg~s}^{-1})$
MS 0451.6-0305	0.540	(1)	1.17	(5)	1371	(7)	10.19	(10)	relatively relaxed	(12)	4
MS 2137.3-2353	0.313	(2)	1.95	(6)	960	(9)	7.97	(10)	relaxed	(13)	5
MS 1008.1-1224	0.3061	(3)	1.18	(5)	1042	(8)	2.29	(10)	non-relaxed	(14)	5
Cl 0412-65	0.507	(4)	0.62	(5)	700	(4)	0.16	(11)			2

References. (1): Donahue (1996b); (2): Stocke et al. (1991); (3): Yee et al. (1998); (4): Dressler et al. (1999); (5): Girardi & Mezzetti (2001); (6): Allen et al. (2003); (7): Carlberg et al. (1996); (8): Borgani et al. (1999); (9): Kneib et al. (1995); (10): Luppino et al. (1999); (11): Smail et al. (1997); (12): Donahue (1996a); (13): Jeltema et al. (2005); (14): Athreya et al. (2002).

Notes. The last column (N) gives the number of galaxies in each cluster that are used in the kinematical analysis.

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