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High-resolution radio observations of GX 339-4

R. P. Fender·R. E. Spencer·S. J. Newell·A. K. Tzioumis
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Abstract

We present radio observations of the black hole candidate X-ray binary GX 339-4 with the Australia Telescope compact array. Mapping of the highest resolution 3.5 cm data reveals a jet-like extension, which if confirmed would be the first detection of a radio jet from a persistent black-hole candidate system. No evidence is found for associated structures such as bow shocks or jet lobes on larger scales. The spectral energy distribution from 22 - 3 cm is relatively flat, suggesting emission is dominated by a compact absorbed core.

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R. P. Fender, R. E. Spencer, S. J. Newell, A. K. Tzioumis. 1997-01-24. High-resolution radio observations of GX 339-4. https://arxiv.org/abs/astro-ph/9701190

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