Co-evolution of black holes and galaxies

被引：0

作者：

Gavignaud, I. ^{[1
,2
]}

Wisotzki, L. ^{[2
]}

Schramm, M. ^{[3
]}

机构：

[1] Univ Andres Bello, Fac Ingn, Dept Ciencias Fis, Santiago, Chile

[2] Astrophysikalisches Inst Postdam, D-14482 Potsdam, Germany

[3] Kyoto Univ, Dept Astron, Kyoto 6068502, Japan

来源：

THIRD ALGERIAN WORKSHOP ON ASTRONOMY AND ASTROPHYSICS | 2010年 / 1295卷

关键词：

galaxies:; actives; VLT DEEP SURVEY; ACTIVE GALACTIC NUCLEI; TYPE-1 AGN SAMPLE; BULGE RELATIONSHIP; HOST GALAXIES; HIGH-REDSHIFT; MASS; LUMINOSITY; QUASARS; DECOMPOSITION;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

One of the most intriguing discoveries of astrophysics in the last decade was to realize that the mass of galactic black holes is tightly correlated to the large scale properties of their host galaxy bulges. The main physical processes at work in shaping this relation is still not clear. One of the main path followed to provide additional constrains to theory is to determine the evolution of the black hole mass - galaxy relation with redshift. I will review in this talk the status in which we are currently standing. I will then report on recent results that we obtained with HST/NICMOS observations of low luminosity host galaxies of z > I AGN. The quality of our data allows us to quantify the contribution of disks to the total stellar-mass of our host galaxies. Our work suggest that the ratio between black-hole mass and bulge stellar-mass was already evolving in the last 9 Gyrs.

引用

页码：117 / +

页数：2

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