Co-Evolution of Supermassive Black Holes and Their Host Galaxies

被引：0

作者：

Kotilainen, J. K. ^{[1
]}

Decarli, R. ^{[2
]}

Falomo, R. ^{[3
]}

Treves, A. ^{[4
]}

Labita, M. ^{[4
]}

Scarpa, R. ^{[5
]}

机构：

[1] Univ Turku, Finnish Ctr Astron ESO FINCA, FI-21500 Turku, Finland

[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany

[3] INAF Osservatorio Astron Padova, I-35122 Padua, Italy

[4] Univ Insubria, I-22100 Como, Italy

[5] Inst Astrofis Canarias, E-38205 Tenerife, Spain

来源：

CO-EVOLUTION OF CENTRAL BLACK HOLES AND GALAXIES | 2010年 / 267期

关键词：

galaxies: active; galaxies: evolution; galaxies: high-redshift; galaxies: nuclei (galaxies:) quasars: general; ACTIVE GALACTIC NUCLEI; QUASI-STELLAR OBJECTS; LUMINOSITY FUNCTION; BULGE RELATIONSHIP; COSMIC EVOLUTION; MASS; SDSS; HISTORY; SIGMA;

D O I：

10.1017/S1743921310005533

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 /M-host relation remains nearly unchanged, taking into account the aging of the stellar population, we find that the M-BH /M-host ratio (Gamma) increases by a factor similar to 7 from z = 0 to z = 3. We show that the evolution of F 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.

引用

页码：34 / +

页数：2

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