The Co-Evolution of Spheroids and Black Holes in the Last 6 Gyrs

Details The Co-Evolution of Spheroids and Black Holes in the Last 6 Gyrs The Co-Evolution of Spheroids and Black Holes in the Last 6 Gyrs

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..399..419w&link_type=abstract

Panoramic Views of Galaxy Formation and Evolution ASP Conference Series, Vol. 399, proceedings of the conference held 11-16 Dece

Astronomy and Astrophysics

Astronomy

Scientific paper

In the present-day universe, the masses of giant black holes correlate with the properties of their host galaxies. This empirical correlation of phenomena on widely different scales suggests that the formation and evolution of galaxies and central black holes are closely linked. I present direct measurements of the correlation between black hole mass and host velocity dispersion of AGN samples at z=0.36 and z=0.57, showing that the relation evolved significantly in the last 6 billion years.

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