The non-ballistic superluminal motion in the plane of the sky-II
Biping Gong, S. W. Kong, F. Xue, Yaping Li, Y. F.Huang

TL;DR
This paper develops a comprehensive non-ballistic jet motion model explaining complex jet morphologies and motions, supported by numerical simulations and unified interpretations of observed phenomena in astrophysical jets.
Contribution
It introduces the first detailed non-ballistic jet model, including simulations and explanations for various jet behaviors and morphologies, bridging gaps in existing models.
Findings
Numerical simulation of multi-knot production in precessing jets
Unified interpretation of bent jets for multi-knot and single knot cases
Explanation for the prevalence of outward motions over inward ones
Abstract
The model of non-ballistic jet motion proposed in 2008 provides a simple explanation to the inward jet motion and bent jet. Recently, evidences of such a non-radial motion increase rapidly, and more complicated morphologies appear. On the other hand, the ballistic plus precession model likely holds in majority samples of jet motion. This paper discusses the relationship between the ballistic and non-ballistic model of jet motion, which suggests that the interaction of ejectors with ambient matter can produce knots at different stages of evolution and hence different separations to the core. And as a jet precesses, knots produced between the core and the deceleration radius result in spiral pattern expected by the model of ballistic plus precession; and knots generated at the deceleration radius display non-radial motion such as bent jet or oscillation of ridge-line. This paper develops…
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