Jet acceleration of the fast molecular outflows in the Seyfert galaxy IC 5063
C. Tadhunter (),
R. Morganti,
M. Rose,
J. B. R. Oonk and
T. Oosterloo
Additional contact information
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
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
Nature, 2014, vol. 511, issue 7510, 440-443
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.
Date: 2014
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Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:511:y:2014:i:7510:d:10.1038_nature13520
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DOI: 10.1038/nature13520
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