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Projekt Druckansicht

The cosmic evolution of the black hole mass / bulge mass ratio

Fachliche Zuordnung Astrophysik und Astronomie
Förderung Förderung von 2007 bis 2012
Projektkennung Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 42000589
 
Erstellungsjahr 2012

Zusammenfassung der Projektergebnisse

We have conducted an extensive study of the statistical properties of the relation between black holes – in particular active ones – and their host galaxies. We determined several important distribution functions characterising the AGN population in the local universe: The z ≈ 0 optical luminosity function of type 1 AGN; the mass function of active black holes and the mass-dependence of the active fraction of black holes; and the distribution of Eddington ratios. These distribution functions are instrumental in order to quantify the inevitable selection biases affecting observations of the important black hole - bulge relations and their evolution with redshift. We developed a new formalism to predict these biases for a specific observational setup and found them to be of similar magnitude and sign as several recently observed trends; we conclude that no statistically significant observational evidence for evolution has yet been detected. In a separate but related study we improved on several black hole masses obtained through stellar dynamical measurements and modelling.

Projektbezogene Publikationen (Auswahl)

 
 

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