Fluctuations and symmetry in the speed and direction of the jets of SS433 on different timescales
Katherine Blundell, Michael Bowler (Oxford), Linda Schmidtobreick, (ESO Santiago)

TL;DR
This study analyzes the speed and directional fluctuations of SS433's jets over different timescales, revealing periodicities, symmetry, and ruling out certain proposed mechanisms, with implications for understanding jet dynamics.
Contribution
It provides new high-resolution spectral data showing jet speed periodicity, symmetry, and anti-correlation between speed and direction, challenging existing models of jet ejection mechanisms.
Findings
Detection of a 13-day periodicity in jet speed.
Jets are highly symmetric on measured timescales.
Anti-correlation between jet speed and direction is confirmed.
Abstract
ABRIDGED We present new results on the variations in speed and direction of the jet bolides in the Galactic microquasar SS433, from high resolution spectra, taken with the ESO 3.6-m New Technology Telescope almost nightly over 0.4 of a precession cycle. We find: (i) These data exhibit multiple ejections within most 24-hour periods and, throughout the duration of the observing campaign, the weighted means of the individual bolides, in both the red jet and the blue jet, clearly exhibit the pronounced nodding known in this system. (ii) We present further evidence for a 13-day periodicity in the jet speed, and show this cannot be dominated by Doppler shifts from orbital motion. (iii) We show the phase of this peak jet speed has shifted by a quarter of a cycle in the last quarter-century. (iv) We show that the two jets ejected by SS433 are highly symmetric on timescales measured thus far.…
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