High-resolution imaging of the molecular outflows in two mergers: IRAS 17208-0014 and NGC 1614
Artikel i vetenskaplig tidskrift, 2015

Context. Galaxy evolution scenarios predict that the feedback of star formation and nuclear activity (AGN) can drive the transformation of gas-rich spiral mergers into (ultra) luminous infrared galaxies and, eventually, lead to the build-up of QSO/elliptical hosts. Aims. We study the role that star formation and AGN feedback have in launching and maintaining the molecular outflows in two starburst-dominated advanced mergers, NGC 1614 (DL = 66 Mpc) and IRAS 17208-0014 (DL = 181 Mpc), by analyzing the distribution and kinematics of their molecular gas reservoirs. Both galaxies present evidence of outflows in other phases of their ISM. Methods. We used the Plateau de Bure interferometer (PdBI) to image the CO(10) and CO(21) line emissions in NGC 1614 and IRAS 17208-0014, respectively, with high spatial resolution (0: 0051: 002). The velocity fields of the gas were analyzed and modeled to find the evidence of molecular outflows in these sources and characterize the mass, momentum, and energy of these components. Results. While most (95%) of the CO emission stems from spatially resolved (23 kpc-diameter) rotating disks, we also detect in both mergers the emission from high-velocity line wings that extend up to -500-700 km s1, well beyond the estimated virial range associated with rotation and turbulence. The kinematic major axis of the line-wing emission is tilted by 90 in NGC 1614 and by 180 in IRAS 17208-0014 relative to the major axes of their respective rotating disks. These results can be explained by the existence of non-coplanar molecular outflows in both systems: the outflow axis is nearly perpendicular to the rotating disk in NGC 1614, but it is tilted relative to the angular momentum axis of the rotating disk in IRAS 17208-0014. Conclusions. In stark contrast to NGC 1614, where star formation alone can drive its molecular outflow, the mass, energy, and momentum budget requirements of the molecular outflow in IRAS 17208-0014 can be best accounted for by the existence of a so far undetected (hidden) AGN of LAGN71011 L The geometry of the molecular outflow in IRAS 17208-0014 suggests that the outflow is launched by a non-coplanar disk that may be associated with a buried AGN in the western nucleus.

Galaxies: ISM

Galaxies: individual: NGC1614

Galaxies: kinematics and dynamics

Galaxies: starburst

Galaxies: nuclei

Galaxies: individual: IRAS 17208-0014

Författare

S. G. Burillo

F. Combes

Centre national de la recherche scientifique (CNRS)

A. Usero

Susanne Aalto

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

L. Colina

Universidad Autonoma de Madrid (UAM)

Centro de Astrobiologia (CAB)

A. Alonso-Herrero

CSIC-UC - Instituto de Física de Cantabria (IFCA)

L. K. Hunt

Osservatorio Astrofisico di Arcetri

S. Arribas

Centro de Astrobiologia (CAB)

Universidad Autonoma de Madrid (UAM)

Francesco Costagliola

CSIC - Instituto de Astrofísica de Andalucía (IAA)

A. Labiano

Eidgenössische Technische Hochschule Zürich (ETH)

R. Neri

Université Grenoble Alpes

M. Pereira-Santaella

Centro de Astrobiologia (CAB)

L. J. Tacconi

Max Planck-institutet

P.P. van der Werf

Universiteit Leiden

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 580 A35

Ämneskategorier

Fusion, plasma och rymdfysik

DOI

10.1051/0004-6361/201526133

Mer information

Senast uppdaterat

2018-09-07