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Article Contents

ABSTRACT

1.INTRODUCTION

2.WHAT SHAPES THE SEDS OF GALAXIES?

3.MODELS WHICH ACCOUNT FOR THE OPTICAL APPEARANCE OF GALAXIES

4.MODELS WHICH ACCOUNT FOR THE ENTIRE OPTICAL/FIR/SUBMM SEDs

4.1.Choice of intrinsic distributions of stars and dust

4.2.Testing the models

4.3.The origin of dust heating

4.4.Application to statistical samples

5.A CLOSER LOOK AT THE ROLE OF CLUMPS IN SHAPING THE SEDS OF GALAXIES

6.MODELLING THE ATTENUATION OF STELLAR LIGHT IN GALAXIES

7.OUTLOOK

REFERENCES