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Twenty Years of Timing SS433
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abstract
We present observations of the optical ``moving lines'' in spectra of the Galactic relativistic jet source SS433 spread over a twenty year baseline from 1979 to 1999. The red/blue-shifts of the lines reveal the apparent precession of the jet axis in SS433, and we present a new determination of the precession parameters based on these data. We investigate the amplitude and nature of time- and phase-dependent deviations from the kinematic model for the jet precession, including an upper limit on any precessional period derivative of $\dot P < 5 \times 10^{-5}$. We also dicuss the implications of these results for the origins of the relativistic jets in SS433.
Forward citations
Cited by 2 Pith papers
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Simulation-based inference for AGN jet population modelling: Towards more robust comparisons of black hole jet speeds
Using neural-posterior-estimation simulation-based inference on the MOJAVE FSRQ sample, the authors infer a Lorentz factor distribution slope b = -1.32 (+0.20, -0.19), consistent with X-ray binary jets at 2 sigma.
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Little Red Dots as Supermassive Analogs of SS 433
LRDs are interpreted as high-inclination hyper-Eddington accreting SMBHs analogous to SS 433, with V-shaped SEDs, X-ray weakness, and Balmer breaks emerging from disk self-shielding geometry.
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