A transient large-scale relativistic radio jet from GX 339-4
Identifieur interne : 00BB19 ( Main/Merge ); précédent : 00BB18; suivant : 00BB20A transient large-scale relativistic radio jet from GX 339-4
Auteurs : E. Gallo [Pays-Bas] ; S. Corbel [France] ; R. P. Fender [Pays-Bas] ; T. J. Maccarone [Pays-Bas] ; A. K. Tzioumis [Australie]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2004.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
We report on the formation and evolution of a large-scale, synchrotron-emitting jet from the black hole candidate and X-ray binary system GX 339-4. In 2002 May, the source moved from a low/hard to a very high X-ray state, contemporaneously exhibiting a very bright optically thin radio flare. Further observations with the Australia Telescope Compact Array have tracked the formation of a collimated structure extending to about 12 arcsec, with apparent velocity greater than 0.9c. The luminosity of the outflow seems to be rapidly decreasing; these observations confirm that transient large-scale jets are likely to be common events triggered by X-ray state transitions in black hole X-ray binaries.
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Pascal:04-0259154Le document en format XML
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<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">A transient large-scale relativistic radio jet from GX 339-4</title>
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<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Accretion disks</term>
<term>Binary X ray source</term>
<term>Black holes</term>
<term>Continuum</term>
<term>Cosmic x-ray sources</term>
<term>Luminosity</term>
<term>Radio stars</term>
<term>Relativistic jet</term>
<term>Transition state</term>
<term>X-ray binary stars</term>
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<keywords scheme="Pascal" xml:lang="fr"><term>Jet relativiste</term>
<term>Trou noir</term>
<term>Binaire RX</term>
<term>Source RX binaire</term>
<term>Luminosité</term>
<term>Etat transition</term>
<term>Disque accrétion</term>
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<term>Continuum</term>
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<front><div type="abstract" xml:lang="en">We report on the formation and evolution of a large-scale, synchrotron-emitting jet from the black hole candidate and X-ray binary system GX 339-4. In 2002 May, the source moved from a low/hard to a very high X-ray state, contemporaneously exhibiting a very bright optically thin radio flare. Further observations with the Australia Telescope Compact Array have tracked the formation of a collimated structure extending to about 12 arcsec, with apparent velocity greater than 0.9c. The luminosity of the outflow seems to be rapidly decreasing; these observations confirm that transient large-scale jets are likely to be common events triggered by X-ray state transitions in black hole X-ray binaries.</div>
</front>
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