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Article Contents
1 Introduction
2 The chemical abundances
3 Characteristic oxygen abundance in spirals as a function of ${M}_{\rm B}$, $V_{\rm rot}$, and Hubble type
4 Comparison between O/H- ${M}_{\rm B}$ relationship for spiral and irregular galaxies
5 The effective oxygen yields
6 Comparison with previous studies
7 Conclusions
Online Material
Appendix A: Distances and luminosities

List of tables
List of figures

Copyright ESO 2004
Published by EDP Sciences