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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.INTERSTELLAR DUST MODELS
- 2.1.What constitutes an
interstellar dust model?
- 2.2.Observational constraints in the
local ISM
- 2.3.Interstellar dust models with cosmic
abundances constraints
- 2.4.Results and astrophysical
implications
- 2.5.Should there be a universal dust
model?
- 3.THE EVOLUTION OF DUST
- 3.1.Dust sources and relative
contributions
- 3.2.Dust processing in the ISM
- 3.3.The destruction of SN condensates by
the reverse shock
- 3.4.Putting it all together in an
idealized evolutionary model
- 4.WHEN DO GALAXIES BECOME FIRST OPAQUE?
- 5.SUMMARY
- REFERENCES