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Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433

Abstract:
SS 433 is a microquasar, a stellar binary system that launches collimated relativistic jets. We observed SS 433 in gamma rays using the High Energy Stereoscopic System (H.E.S.S.) and found an energy-dependent shift in the apparent position of the gamma-ray emission from the parsec-scale jets. These observations trace the energetic electron population and indicate that inverse Compton scattering is the emission mechanism of the gamma rays. Our modeling of the energy-dependent gamma-ray morphology constrains the location of particle acceleration and requires an abrupt deceleration of the jet flow. We infer the presence of shocks on either side of the binary system, at distances of 25 to 30 parsecs, and that self-collimation of the precessing jets forms the shocks, which then efficiently accelerate electrons.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1126/science.adi2048

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Grant:
ST/X001598/1
ST/M00757X/1
ST/S002618/1
ST/V001477/1
ST/S002952/1
ST/L006499/1
ST/V006355/1
ST/W508019/1


Publisher:
American Association for the Advancement of Science
Journal:
Science More from this journal
Volume:
383
Issue:
6681
Pages:
402-406
Place of publication:
United States
Publication date:
2024-01-25
Acceptance date:
2023-12-04
DOI:
EISSN:
1095-9203
ISSN:
0036-8075
Pmid:
38271522


Language:
English
Keywords:
Pubs id:
1607326
Local pid:
pubs:1607326
Deposit date:
2024-01-28

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