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Fig. 7.

image

Model of the source geometry in S5 0836+710 as an FR II radio galaxy observed at a small inclination angle θ. HS denotes the hotspot region closer to the observer, and CHS denotes the counter-hotspot region. The different arm lengths are due to the different light travel times (see Appendix A). The two jets are misaligned by φ from a straight jet/counter-jet axis.

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