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Gas inflow and AGN-driven outflow in M51

Published online by Cambridge University Press:  09 February 2015

M. Querejeta ,
S. E. Meidt ,
E. Schinnerer ,
S. García-Burillo ,
J. Pety ,
A. Hughes ,
D. Meier ,
F. Bigiel ,
K. Kreckel  and
G. Blanc
M. Querejeta
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: querejeta@mpia.de
S. E. Meidt
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: querejeta@mpia.de
E. Schinnerer
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: querejeta@mpia.de
S. García-Burillo
Affiliation:
OAN, Madrid, Spain
J. Pety
Affiliation:
IRAM, Grenoble, France
A. Hughes
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: querejeta@mpia.de
D. Meier
Affiliation:
New Mexico Tech, USA
F. Bigiel
Affiliation:
University of Heidelberg, Germany
K. Kreckel
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: querejeta@mpia.de
G. Blanc
Affiliation:
Carnegie Institution, USA.
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Abstract

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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.

Keywords

galaxies: AGN — galaxies: structure — galaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 338
Copyright
Copyright © International Astronomical Union 2015