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Images of an equatorial outflow in SS433

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arxiv astro-ph/0109504 v1 pith:5HBVV6JK submitted 2001-09-27 astro-ph

classification astro-ph
keywords binaryemissionoutflowsmoothss433systemvlbaappearance
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We have imaged the X-ray binary SS433 with unprecedented Fourier-plane coverage at 6cm using simultaneously the VLBA, MERLIN, and the VLA, and also at 20cm with the VLBA. At both wavelengths we have securely detected smooth, low-surface brightness emission having the appearance of a `ruff' or collar attached perpendicularly to the well-studied knotty jets in this system, extending over at least a few hundred AU. We interpret this smooth emission as a wind-like outflow from the binary, and discuss its implications for the present evolutionary stage of this system.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Distinct Jet Properties in the X-Ray-Obscured State of GRS 1915+105

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    VLBI observations during 2025 radio flares find no detectable jet motion in GRS 1915+105, implying its obscured-state jets are slower (βΓ≲0.40) than the pre-2019 relativistic jets.

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