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Article Contents
1 Introduction
2 The galaxy sample and complementary data
3 $\vec{L}_{{\rm C~II}}/\vec{L}_{{\rm FIR}}$ vs. H $\alpha~{\vec {EW}}$ in normal late-type galaxies
4 The model
5 Results
6 Discussion
7 Conclusions
References

Copyright ESO 2003
Published by EDP Sciences