Abstract
A numerical model is used to follow the two-dimensional shell of a three-dimensional radio jet. This model, in the spirit of previous work of Wiita and Siah, invokes a new computer code to allow internal pressure of the jet fluid to be taken as a tensor, allowing for bulk motion of the internal relativistic gas and azimuthal symmetry is no longer assumed. Three-dimensional effects of two kinds have been modeled: bending in a “wind” resulting from motion of the host galaxy through an intergalactic medium; and stability of the beam cross-sectional shape.
Results of the two-dimensional cases confirm and strengthen earlier inferences that hydrodynamics alone is incapable of accounting for observed jet collimation. Results on jet bending suggest, once again, that non-hydrodynamic effects must be invoked to explain some observations. With respect to beam cross-section, intricate oscillatory motions have been observed, some of which appear to be unstable and potentially disruptive.
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© 1988 Springer-Verlag
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Mitteldorf, J., Wiita, P.J. (1988). Two-and-one-half dimensional models of radio jets. In: Miller, H.R., Wiita, P.J. (eds) Active Galactic Nuclei. Lecture Notes in Physics, vol 307. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-19492-4_227
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DOI: https://doi.org/10.1007/3-540-19492-4_227
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