S5 0836+710: An FRII jet disrupted by the growth of a helical instability?
M. PeruchoDept. d’Astronomia i Astrofísica, Universitat de València, C/ Dr. Moliner 50, 46100 Burjassot (València), SpainI. Martí-VidalOnsala Space Observatory (Chalmers University of Technology), Observatorievägen 90, 43992 Onsala, SwedenA. P. LobanovMax-Planck-Institut für Radioastronomie (MPIfR), Auf dem Hügel 69, 53121 Bonn, GermanyP. E. HardeeDepartment of Physics & Astronomy, The University of Alabama, Tuscaloosa, AL 35487, USA
2012en
ABI
Аннотация
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.
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