Table A.2: Same as Table A.1 but for the H II regions of NGC 1530.
Cut-off for log $L_{{\rm H}\alpha}>38.4$ for log $L_{{\rm H}\alpha}>38.8$ Complet.

isophote slope stdev slope stdev limit

$I_{\rm peak}/e$ 2.2 0.2 2.4 0.3 38.2

0.5 $I_{\rm peak}$ 2.3 0.3 2.6 0.5 38.1

3 rms 2.0 0.2 2.1 0.6 38.2

5 rms 2.9 0.4 2.5 0.4 38.4

7 rms 3.3 0.5 2.4 0.7 38.5

**Table A.2:** Same as Table A.1 but for the H II regions of NGC 1530.
Cut-off	for log $L_{{\rm H}\alpha}>38.4$	for log $L_{{\rm H}\alpha}>38.8$	Complet.
isophote	slope	stdev	slope	stdev	limit
$I_{\rm peak}/e$	2.2	0.2	2.4	0.3	38.2
0.5 $I_{\rm peak}$	2.3	0.3	2.6	0.5	38.1
3 rms	2.0	0.2	2.1	0.6	38.2
5 rms	2.9	0.4	2.5	0.4	38.4
7 rms	3.3	0.5	2.4	0.7	38.5

Source LaTeX | All tables | In the text

	1 Introduction
	2 The observations
	3 Relating the photometric and spectroscopic data sets
	4 Extraction of the line profiles
	5 Spectral analysis
	6 The luminosity v. non-thermal velocity dispersion relation
	7 The masses of the H II regions in the log L ${_{\scriptsize {\rm H \alpha}}}$ - log ${\sigma _{\rm nt}}$ diagram
	8 Conclusions
	Appendix A: The effects of different H II region size estimate criteria
	References