To appear in the proceedings of the 2011 Frank N. Bash Symposium, "New Horizons in Astronomy".
astro-ph/1206.2661

For a PDF version of the article, click here.

BLACK HOLE -- GALAXY CO-EVOLUTION

Kevin Schawinski


Einstein Fellow
Department of Physics, Yale University, New Haven, CT 06511, U.S.A.
Yale Center for Astronomy and Astrophysics, Yale University, P.O. Box 208121, New Haven, CT 06520, U.S.A.


Table of Contents

WHY CO-EVOLUTION?

EVIDENCE FOR CO-EVOLUTION

MULTIPLE MODES OF CO-EVOLUTION
The Local Universe
Early-type AGN Host Galaxies - Merger-driven Migration from Blue to Red
Late-type AGN Host Galaxies - Secular Evolution and Stochastic Feeding
The High Redshift Universe

ACCRETION STATES AND TRANSITIONS

OPEN QUESTIONS & PROSPECTS

REFERENCES

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