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- W2100060802 abstract "Abstract We study the evolution of the M BH / M host relation up to z = 3 for a sample of 96 quasars with known host galaxy luminosities. Black hole masses are estimated assuming virial equilibrium in the broad-line regions, while the host galaxy masses are inferred from their luminosities. With this data, we are able to pin down the evolution of the M BH / M host relation over 85% of the age of the universe. While the M BH / L host relation remains nearly unchanged, taking into account the aging of the stellar population, we find that the M BH / M host ratio (Γ) increases by a factor ~ 7 from z = 0 to z = 3. We show that the evolution of Γ is independent of radio loudness and quasar luminosity. We propose that the most massive black holes, in their quasar phase at high-redshift, become extremely rare objects in host galaxies of similar mass in the local universe." @default.
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- W2100060802 date "2009-08-01" @default.
- W2100060802 modified "2023-09-27" @default.
- W2100060802 title "Co-Evolution of Supermassive Black Holes and Their Host Galaxies" @default.
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- W2100060802 doi "https://doi.org/10.1017/s1743921310005533" @default.
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