Table 3: The derived global characteristics of BCDGs compared with the Salzer et al. (2002) sample.
BCDG sample Salzer sample

median min max median min max

A₀ [kpc] 3.1 1.0 7.5 3.2 0.5 11

M_B -15.5 -12.4 -17.4 -16.1 -12 -17.5

$M_{{\rm HI}}$ [10 $^{8}~M_{\odot}]$ 1.5 0.9 14.5 3.0 0.2 18

W₅₀ [km s^-1] 58 29 190 88 30 220

**Table 3:** The derived global characteristics of BCDGs compared with the Salzer et al. (2002) sample.
	BCDG sample	Salzer sample
	median	min	max	median	min	max
A₀ [kpc]	3.1	1.0	7.5	3.2	0.5	11
M_B	-15.5	-12.4	-17.4	-16.1	-12	-17.5
$M_{{\rm HI}}$ [10 $^{8}~M_{\odot}]$	1.5	0.9	14.5	3.0	0.2	18
W₅₀ [km s^-1]	58	29	190	88	30	220

Source LaTeX | All tables | In the text

	1 Introduction
	2 The sample of BCDGs
	3 H I-observations
	4 The basic results
	5 Comments on individual galaxies
	6 Discussion
	References