The precession of SS433's radio ruff on long timescales
S. Doolin, K. M. Blundell

TL;DR
This paper investigates the changing orientation of SS433's radio-emitting plasma outflow, called the ruff, over long timescales, proposing that circumbinary disk dynamics cause its precession, supported by 3D numerical simulations.
Contribution
The study links the ruff's reorientation to circumbinary orbit precession, providing a new explanation supported by numerical simulations matching observed precession rates.
Findings
Ruff reorientation is not coupled with jet precession.
Circumbinary orbits can precess in longitude of the ascending node.
Matching observed precession requires specific binary parameters.
Abstract
Roughly perpendicular to SS433's famous precessing jets is an outflowing "ruff" of radio-emitting plasma, revealed by direct imaging on milli-arcsecond scales. Over the last decade, images of the ruff reveal that its orientation changes over time with respect to a fixed sky co-ordinate grid. For example, during two months of daily observations with the VLBA by Mioduszewski et al. (2004), a steady rotation through ~10 degrees is observed whilst the jet angle changes by ~20 degrees. The ruff reorientation is not coupled with the well-known precession of SS433's radio jets, as the ruff orientation varies across a range of 69 degrees whilst the jet angle varies across 40 degrees, and on greatly differing and non-commensurate timescales. It has been proposed that the ruff is fed by SS433's circumbinary disk, discovered by a sequence of optical spectroscopy by Blundell et al. (2008), and so…
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