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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S309(10), p. 338-338

DOI: 10.1017/s174392131401031x

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Gas inflow and AGN-driven outflow in M51

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe 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.

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