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Gas inflow and AGN-driven outflow in M51

Published online by Cambridge University Press:  09 February 2015

M. Querejeta
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: [email protected]
S. E. Meidt
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: [email protected]
E. Schinnerer
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: [email protected]
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: [email protected]
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: [email protected]
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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015