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Article Contents

ABSTRACT

1.INTRODUCTION

2.GRAIN MODELS

3.FIRST ATTEMPTS TO EXPLAIN THE INFRARED SPECTRA OF IRAS GALAXIES

4.THE DESTRUCTION OF VERY SMALL GRAINS

5.TOWARDS A NEW PICTURE OF INTERSTELLAR DUST IN GALAXIES

6.FAR INFRARED AND SUBMILLIMETRE MAPPING OF GALAXIES

7.DETERMINATION OF DUST MASS IN GALAXIES

8.DUST IN ELLIPTICALS AND LENTICULARS

REFERENCES