Accretion of stellar winds in the galactic centre

被引：0

作者：

Cuadra, J. ^{[1
]}

Nayakshin, S. ^{[1
,2
]}

Springel, V. ^{[1
]}

Di Matteo, T. ^{[1
,3
]}

机构：

[1] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany

[2] Univ Leicester, Leicester LE1 7RH, Leics, England

[3] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA

来源：

XI IAU REGIONAL LATIN AMERICAN MEETING OF ASTRONOMY | 2006年 / 26卷

关键词：

accretion; accretion discs; galaxy : center; stars; winds; outflows;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Sgr A* is identified with the M-BH similar to 3.5 x 10(6)M(circle dot) super-massive black hole (SMBH) at the centre of our Galaxy. By virtue of its proximity, Sgr A* may play a key role in the understanding of Active Galactic Nuclei (AGN). Indeed, this is the only AGN where observations detail the origin of the gas in the vicinity of the SMBH. This information is absolutely necessary for the accretion problem to be modelled self-consistently.

引用

页码：139 / +

页数：2

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