Table 5: General H I properties.
NGC 1406 NGC 1511 NGC 4244 NGC 4565 NGC 4666^a NGC 4700 NGC 7090 NGC 7462

$\alpha$ (2000)^b 03:39:22.8 03:59:36.9 12:17:29.9 12:36:21.0 12:45:08.3 12:49:07.6 21:36:28.6 23:02:46.5

$\delta$ (2000)^b -31:19:16 -67:38:08 +37:48:31 +25:59:13 -00:27:51 -11:24:47 -54:33:24 -40:50:05

D (Mpc)^c 14.9 17.5 3.0 9.7^d 26.4 25.5 11.7 15.1

$v_{\rm hel}$ (km s^-1) 1051 1335 244 1221 1520 1404 849 1064

PA ( $^\circ$ ) 199 295 228 315 225 48 130 253

i ( $^\circ$ ) 90^e 72^e 84.5^f $\geq$ 87.5^g 70 90^e 90^e 90^e

$v_{\rm max}$ (km s^-1) 171 150 113 271 180 87 124 112

$v_{\rm max}^{\rm i}$ (km s^-1) 171 158 114 271 192 87 124 112

R₀ (kpc) 4.1 4.9 4.7 4.8 17 5.6 5.7 4.5

$f_{\rm HI}$ (Jy km s^-1) 62.3 44.3 379 249 93.5 21.7 39.8 32.7

$M_{\rm atom}$ (10⁹ $M_{\odot}$ ) 4.40 4.32 1.09 7.45 15.3 4.48 1.73 2.37

Notes (for details see text):
^a Values from Walter et al. (2004).
^b The kinematic centre positions were determined from rotation curve fitting using routine ROTCUR in GIPSY (see text).
^c Distances are based on H₀ = 75 Mpc km s^-1 and a virgocentric infall velocity of 300 km s^-1 (cf. Dahlem et al. 2001).
^d The distance of NGC 4565 is hard to determine because of the peculiar velocities of the Coma clouds (Ferrarese et al. 2000). The value used here is from Tully (1988).
^e Tully (1988).
^f Olling (1996a).
^g Rupen (1991).

**Table 5:** General H I properties.
	NGC 1406	NGC 1511	NGC 4244	NGC 4565	NGC 4666^a	NGC 4700	NGC 7090	NGC 7462
$\alpha$ (2000)^b	03:39:22.8	03:59:36.9	12:17:29.9	12:36:21.0	12:45:08.3	12:49:07.6	21:36:28.6	23:02:46.5
$\delta$ (2000)^b	-31:19:16	-67:38:08	+37:48:31	+25:59:13	-00:27:51	-11:24:47	-54:33:24	-40:50:05
D (Mpc)^c	14.9	17.5	3.0	9.7^d	26.4	25.5	11.7	15.1
$v_{\rm hel}$ (km s^-1)	1051	1335	244	1221	1520	1404	849	1064
PA ( $^\circ$ )	199	295	228	315	225	48	130	253
i ( $^\circ$ )	90^e	72^e	84.5^f	$\geq$ 87.5^g	70	90^e	90^e	90^e
$v_{\rm max}$ (km s^-1)	171	150	113	271	180	87	124	112
$v_{\rm max}^{\rm i}$ (km s^-1)	171	158	114	271	192	87	124	112
R₀ (kpc)	4.1	4.9	4.7	4.8	17	5.6	5.7	4.5
$f_{\rm HI}$ (Jy km s^-1)	62.3	44.3	379	249	93.5	21.7	39.8	32.7
$M_{\rm atom}$ (10⁹ $M_{\odot}$ )	4.40	4.32	1.09	7.45	15.3	4.48	1.73	2.37

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Results
	4 Discussion
	References
	Online Material
	Appendix A: New 1.4 GHz radio continuum images