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Molecular Outflows in Galaxy Merger Simulations with Embedded Active Galactic Nuclei

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Published 2006 April 24 © 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Desika Narayanan et al 2006 ApJ 642 L107 DOI 10.1086/504846

1538-4357/642/2/L107

Abstract

We study the effects of feedback from active galactic nuclei (AGNs) on emission from molecular gas in galaxy mergers by combining hydrodynamic simulations that include black holes with a three-dimensional, non-local thermodynamic equilibrium (LTE) radiative transfer code. We find that molecular clouds entrained in AGN winds produce an extended CO morphology with significant off-nuclear emission, which may be detectable via contour mapping. Furthermore, kinematic signatures of these molecular outflows are visible in emission-line profiles when the outflow has a large line-of-sight velocity. Our results can help interpret current and upcoming observations of luminous infrared galaxies, as well as provide a detailed test of subresolution prescriptions for supermassive black hole growth in galaxy-scale hydrodynamic simulations.

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10.1086/504846