AustralieFrV1, Main, Exploration, bibRecord, 00B661

Large-scale, decelerating, relativistic X-ray jets from the microquasar XTE J1550-564

Identifieur interne : 00B661 ( Main/Exploration ); précédent : 00B660; suivant : 00B662

Large-scale, decelerating, relativistic X-ray jets from the microquasar XTE J1550-564

Auteurs : S. Corbel [France] ; R. P. Fender [États-Unis] ; A. K. Tzioumis [Australie] ; J. A. Tomsick [États-Unis] ; J. A. Orosz [Pays-Bas] ; J. M. Miller [États-Unis] ; R. Wijnands [États-Unis] ; P. Kaaret [États-Unis]

Source :

Science : (Washington, D.C.) [ 0036-8075 ] ; 2002.

RBID : Pascal:02-0581980

Descripteurs français

Pascal (Inist)
- Source RX galactique, Source RX transitoire, Jet galactique, Jet relativiste, Décélération, Evolution dynamique, Voie lactée, Trou noir, Binaire RX, Rayonnement synchrotron.

English descriptors

KwdEn :
- Black holes, Deceleration, Dynamical evolution, Galactic X ray source, Galactic jet, Milky Way, Relativistic jet, Synchrotron radiation, Transient X ray source, X-ray binary stars.

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 teraelectron 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.

Affiliations:

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Le document en format XML

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<front><div type="abstract" xml:lang="en">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 teraelectron 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.</div>
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<country name="Pays-Bas"><region name="Utrecht (province)"><name sortKey="Orosz, J A" sort="Orosz, J A" uniqKey="Orosz J" first="J. A." last="Orosz">J. A. Orosz</name>
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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

Source :

Descripteurs français

English descriptors

Abstract

Links toward previous steps (curation, corpus...)

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

Pour mettre un lien sur cette page dans le réseau Wicri