SS 433: Flares and L2 Overflow Spirals

Author:

Bowler Michael1

Affiliation:

1. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK

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 L2 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. It also provides a new measure of the mass ratio of the binary.

Publisher

MDPI AG

Reference12 articles.

1. SS 433: Two robust determinations fix the mass ratio;Bowler;Astron. Astrophys.,2018

2. Bowler, M.G. (2020). SS 433: C II emission from the disk photosphere. arXiv.

3. HESS Collaboration, Aharonian, F., Benkhali, F.A., Aschersleben, J., Ashkar, H., Backes, M., Martins, V.B., Batzofin, R., Becherini, Y., and Berge, D. (2024). Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433. Science, 383, 402–406.

4. W50 and SS 433;Bowler;Astron. Astrophys.,2018

5. Bowler, M.G. (2024). W50 morphology and the dynamics of SS 433 formation. arXiv.

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