Article
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SS 433: Flares and L2 Overflow, Spirals in the Wind
Version 1
: Received: 17 June 2024 / Approved: 18 June 2024 / Online: 18 June 2024 (08:16:00 CEST)
How to cite: Bowler, M. SS 433: Flares and L2 Overflow, Spirals in the Wind. Preprints 2024, 2024061194. https://doi.org/10.20944/preprints202406.1194.v1 Bowler, M. SS 433: Flares and L2 Overflow, Spirals in the Wind. Preprints 2024, 2024061194. https://doi.org/10.20944/preprints202406.1194.v1
Abstract
Flaring in the SS 433 microquasar is dominated by outbursts from material at distances from the centre of mass of the binary system comparable to the separation of the two components. This note completes a demonstration that ejected plasma leaves the system in the region of the L_2 point, there overflowing the outer Roche lobe and giving rise to a spiral structure as it leaves the system as part of the local environment.
Keywords
X-rays: binaries: ULX; stars: binaries: SS 433; galaxies: stellar content: microquasar
Subject
Physical Sciences, Astronomy and Astrophysics
Copyright: This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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