Volume 545, September 2012
|Number of page(s)||4|
|Published online||05 September 2012|
S5 0836+710: An FRII jet disrupted by the growth of a helical instability?⋆
1 Dept. d’Astronomia i Astrofísica, Universitat de València,
C/ Dr. Moliner 50, 46100 Burjassot (València), Spain
2 Onsala Space Observatory (Chalmers University of Technology), Observatorievägen 90, 43992 Onsala, Sweden
3 Max-Planck-Institut für Radioastronomie (MPIfR), Auf dem Hügel 69, 53121 Bonn, Germany
4 Department of Physics & Astronomy, The University of Alabama, Tuscaloosa, AL 35487, USA
Received: 8 June 2012
Accepted: 25 July 2012
Context. The remarkable stability of extragalactic jets is surprising, given the reasonable possibility of the growth of instabilities. In addition, much work in the literature has invoked this possibility to explain observed jet structures and obtain information about the jet from these structures. For example, it has been shown that the observed helical structures in the jet in S5 0836+710 could be associated with helical pressure waves generated by a Kelvin-Helmholtz instability.
Aims. Our aim is to resolve the arc-second structure of the jet in the quasar S5 0836+710 and confirm the lack of a hot-spot (reverse jet-shock) found by present observing arrays, as this lack implies a loss of jet collimation before interaction with the intergalactic medium.
Methods. We use an observation performed in 2008 using EVN (European Very Long Baseline Interferometry Network) and MERLIN (Multi-Element Radio Linked Interferometer Network). The resultant combined image after data reduction has provided a complete image of the object on arc-second scales.
Results. The lack of a hot-spot in the arc-second radio structure is taken as evidence that the jet loses its collimation between the VLBI (Very Long Baseline Interferometry) region and the region of interaction with the ambient medium.
Conclusions. This result and the previous identification of the helical structures in the jet with helical pressure waves that grow in amplitude with distance allow us to conclude that the jet is probably disrupted by the growth of Kelvin-Helmholtz instability. This observational evidence confirms that the physical parameters of jets can be extracted using the assumption that instability is present in jets and can be the reason for many observed structures. Interestingly, the observed jet is classified as a FRII (Fanaroff-Riley type II) object in terms of its luminosity, but its large-scale morphology does not correspond to this classification. The implications of this finding are discussed.
Key words: galaxies: jets / hydrodynamics / instabilities / quasars: individual: S5 0836+710
FITS files are available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (188.8.131.52) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/545/A65
© ESO, 2012
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