AustralieFrV1, Main, Exploration, bibRecord, 00A965

A transient large‐scale relativistic radio jet from GX 339−4

Identifieur interne : 00A965 ( Main/Exploration ); précédent : 00A964; suivant : 00A966

A 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 ] ; 2004-01.

RBID : ISTEX:DB955C5E8B856326409CD1372BE9D6FB31835E45

Descripteurs français

Pascal (Inist)
- Binaire RX, Continuum, Disque accrétion, Etat transition, Etoile radio, Jet relativiste, Luminosité, Source RX binaire, Source RX cosmique, Trou noir.
Wicri :
- topic : Niveau sonore.

English descriptors

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.

Url:

DOI: 10.1111/j.1365-2966.2004.07435.x

Affiliations:

Le document en format XML

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<term>Lower limit</term>
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<term>Minimum velocity</term>
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<term>Mnras</term>
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<term>Position angles</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>
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A transient large‐scale relativistic radio jet from GX 339−4

A transient large‐scale relativistic radio jet from GX 339−4

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Descripteurs français

English descriptors

Abstract

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