SwePub
Sök i LIBRIS databas

  Extended search

(WFRF:(Labiano A.))
 

Search: (WFRF:(Labiano A.)) > (2015-2019) > High-resolution ima...

  • Burillo, S. G. (author)

High-resolution imaging of the molecular outflows in two mergers: IRAS 17208-0014 and NGC 1614

  • Article/chapterEnglish2015

Publisher, publication year, extent ...

  • 2015-07-23
  • EDP Sciences,2015
  • electronicrdacarrier

Numbers

  • LIBRIS-ID:oai:research.chalmers.se:b280ff0a-14b4-48d9-a8e2-9405462edda0
  • https://doi.org/10.1051/0004-6361/201526133DOI
  • https://research.chalmers.se/publication/220959URI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

  • Subject category:art swepub-publicationtype
  • Subject category:ref swepub-contenttype

Notes

  • 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.

Subject headings and genre

Added entries (persons, corporate bodies, meetings, titles ...)

  • Combes, F.Centre national de la recherche scientifique (CNRS) (author)
  • Usero, A. (author)
  • Aalto, Susanne,1964Chalmers tekniska högskola,Chalmers University of Technology(Swepub:cth)saalto (author)
  • Colina, L.Centro de Astrobiologia (CAB),Universidad Autonoma de Madrid (UAM) (author)
  • Alonso-Herrero, A.CSIC-UC - Instituto de Física de Cantabria (IFCA) (author)
  • Hunt, L. K.Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory (author)
  • Arribas, S.Centro de Astrobiologia (CAB),Universidad Autonoma de Madrid (UAM) (author)
  • Costagliola, Francesco,1981Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)(Swepub:cth)costagli (author)
  • Labiano, A.Eidgenössische Technische Hochschule Zürich (ETH),Swiss Federal Institute of Technology in Zürich (ETH) (author)
  • Neri, R.Université Grenoble Alpes,Grenoble Alpes University (author)
  • Pereira-Santaella, M.Centro de Astrobiologia (CAB) (author)
  • Tacconi, L. J.Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG) (author)
  • van der Werf, P.P.Universiteit Leiden (UL),Leiden University (UL) (author)
  • Centre national de la recherche scientifique (CNRS)Chalmers tekniska högskola (creator_code:org_t)

Related titles

  • In:Astronomy and Astrophysics: EDP Sciences5800004-63611432-0746

Internet link

Find in a library

To the university's database

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view