Gas inflow and AGN-driven outflow in M51

被引：0

作者：

Querejeta, M. ^{[1
]}

Meidt, S. E. ^{[1
]}

Schinnerer, E. ^{[1
]}

Garcia-Burillo, S. ^{[2
]}

Pety, J. ^{[3
]}

Hughes, A. ^{[1
]}

Meier, D. ^{[4
]}

Bigiel, F. ^{[5
]}

Kreckel, K. ^{[1
]}

Blanc, G. ^{[6
]}

机构：

[1] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[2] OAN, Madrid, Spain

[3] IRAM, Grenoble, France

[4] New Mexico Inst Min & Technol, Socorro, NM USA

[5] Heidelberg Univ, Heidelberg, Germany

[6] Carnegie Inst, Washington, DC USA

来源：

GALAXIES IN 3D ACROSS THE UNIVERSE | 2014年 / 10卷 / 309期

关键词：

galaxies: AGN; galaxies: structure; galaxies: evolution;

D O I：

10.1017/S174392131401031X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study the feeding and feedback of the nucleus of M51 by considering gravitational torques, responsible for gas inflow, in relation to the local distribution of dense gas.

引用

页码：338 / 338

页数：1