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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.OBSERVATIONAL CONSTRAINTS ON
INTERSTELLAR DUST
- 3.WARM AND COLD DUST IN THE ISM
- 4.THE SILICATE-GRAPHITE-PAHS INTERSTELLAR
DUST MODEL
- 5.VERY COLD DUST OR HOW COLD COULD
GALAXIES BE?
- 6.CAN DUST GET DOWN TO 2.7 K AND APPEAR IN
ABSORPTION AGAINST THE CMB?
- 7.NOTES
- REFERENCES