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Jet acceleration of the fast molecular outflows in the Seyfert galaxy IC 5063

Author

Listed:
  • C. Tadhunter

    (University of Sheffield, Sheffield S3 7RH, UK)

  • R. Morganti

    (ASTRON, The Netherlands Institute of Radio Astronomy, PO Box 2, 7990 AA, Dwingeloo, The Netherlands
    Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands)

  • M. Rose

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street)

  • J. B. R. Oonk

    (ASTRON, The Netherlands Institute of Radio Astronomy, PO Box 2, 7990 AA, Dwingeloo, The Netherlands)

  • T. Oosterloo

    (ASTRON, The Netherlands Institute of Radio Astronomy, PO Box 2, 7990 AA, Dwingeloo, The Netherlands
    Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands)

Abstract

The observation of high-velocity warm molecular hydrogen in the galaxy IC 5063 supports the proposal that the powerful jets of particles launched by active galactic nuclei can both accelerate and heat the molecular outflows that influence the evolution of galaxies.

Suggested Citation

  • C. Tadhunter & R. Morganti & M. Rose & J. B. R. Oonk & T. Oosterloo, 2014. "Jet acceleration of the fast molecular outflows in the Seyfert galaxy IC 5063," Nature, Nature, vol. 511(7510), pages 440-443, July.
    • Handle: RePEc:nat:nature:v:511:y:2014:i:7510:d:10.1038_nature13520
    DOI: 10.1038/nature13520
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