Large-scale, decelerating, relativistic X-ray jets from the microquasar XTE J1550-564
Large-scale, decelerating, relativistic X-ray jets from the microquasar XTE J1550-564
We have detected, at x-ray and radio wavelengths, large-scale moving jets from the microquasar XTE J1550-564. Plasma ejected from near the black hole traveled at relativistic velocities for at least 4 years. We present direct evidence for gradual deceleration in a relativistic jet. The broadband spectrum of the jets is consistent with synchrotron emission from high-energy (up to 10 tera-electron volts) particles that were accelerated in the shock waves formed within the relativistic ejecta or by the interaction of the jets with the interstellar medium. XTE J1550-564 offers a rare opportunity to study the dynamical evolution of relativistic jets on time scales inaccessible for active galactic nuclei jets, with implications for our understanding of relativistic jets from Galactic x-ray binaries and active galactic nuclei.
196-199
Corbel, S.
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Fender, R.P.
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Tzioumis, A.K.
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Tomsick, J.A.
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Orosz, J.A.
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Miller, J.M.
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Wijnands, R.
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Kaaret, P.
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4 October 2002
Corbel, S.
b31cdd54-9e1c-4bfa-ac85-f98c627ff455
Fender, R.P.
c802ddfc-25a3-4c0e-899d-11c405c705d1
Tzioumis, A.K.
d069871e-6e05-4f5a-a876-58fc583346c6
Tomsick, J.A.
a9cc3ecb-ac1b-4561-8570-edf46d54cd2f
Orosz, J.A.
a4dd6086-9663-445c-88d7-4899aa26cd57
Miller, J.M.
078305f0-03c7-4982-95ff-a92bc2f75b54
Wijnands, R.
382893ee-0e03-45e3-9321-db8b9fc74914
Kaaret, P.
033c5643-89d8-4af0-83da-3a6c032bcfd3
Corbel, S., Fender, R.P., Tzioumis, A.K., Tomsick, J.A., Orosz, J.A., Miller, J.M., Wijnands, R. and Kaaret, P.
(2002)
Large-scale, decelerating, relativistic X-ray jets from the microquasar XTE J1550-564.
Science, 298 (5991), .
(doi:10.1126/science.1075857).
Abstract
We have detected, at x-ray and radio wavelengths, large-scale moving jets from the microquasar XTE J1550-564. Plasma ejected from near the black hole traveled at relativistic velocities for at least 4 years. We present direct evidence for gradual deceleration in a relativistic jet. The broadband spectrum of the jets is consistent with synchrotron emission from high-energy (up to 10 tera-electron volts) particles that were accelerated in the shock waves formed within the relativistic ejecta or by the interaction of the jets with the interstellar medium. XTE J1550-564 offers a rare opportunity to study the dynamical evolution of relativistic jets on time scales inaccessible for active galactic nuclei jets, with implications for our understanding of relativistic jets from Galactic x-ray binaries and active galactic nuclei.
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Published date: 4 October 2002
Identifiers
Local EPrints ID: 40533
URI: http://eprints.soton.ac.uk/id/eprint/40533
ISSN: 0036-8075
PURE UUID: 723ba57f-bfe4-4c0e-af10-556dd265423e
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Date deposited: 04 Jul 2006
Last modified: 15 Mar 2024 08:20
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Contributors
Author:
S. Corbel
Author:
R.P. Fender
Author:
A.K. Tzioumis
Author:
J.A. Tomsick
Author:
J.A. Orosz
Author:
J.M. Miller
Author:
R. Wijnands
Author:
P. Kaaret
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