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Article Contents

ABSTRACT

1.WHY CO-EVOLUTION?

2.EVIDENCE FOR CO-EVOLUTION

3.MULTIPLE MODES OF CO-EVOLUTION

3.1.The Local Universe

3.2.Early-type AGN Host Galaxies - Merger-driven Migration from Blue to Red

3.3.Late-type AGN Host Galaxies - Secular Evolution and Stochastic Feeding

3.4.The High Redshift Universe

4.ACCRETION STATES AND TRANSITIONS

5.OPEN QUESTIONS & PROSPECTS

REFERENCES