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A transient large-scale relativistic radio jet from GX 339-4

Identifieur interne : 00BB19 ( Main/Merge ); précédent : 00BB18; suivant : 00BB20

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 :

RBID : Pascal:04-0259154

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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:04-0259154

Le document en format XML

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