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Molecular outflows in galaxy merger simulations with embedded active galactic nuclei

  • Desika Narayanan
  • , Thomas J. Cox
  • , Brant Robertson
  • , Romeel Davé
  • , Tiziana D.I. Matteo
  • , Lars Hernquist
  • , Philip Hopkins
  • , Craig Kulesa
  • , Christopher K. Walker

Research output: Contribution to journalArticlepeer-review

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.

Original languageEnglish (US)
Pages (from-to)L107-L110
JournalAstrophysical Journal
Volume642
Issue number2 II
DOIs
StatePublished - May 10 2006

Keywords

  • Cosmology: theory
  • Galaxies: ISM
  • Galaxies: active
  • Galaxies: formation
  • Galaxies: interactions
  • Line: formation

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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