High-resolution radio observations of GX 339-4

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dc.creatorFender, R. P.
dc.creatorSpencer, R. E.
dc.creatorNewell, S. J.
dc.creatorTzioumis, A. K.
dc.date1997-01-24
dc.date.accessioned2026-07-07T02:22:48Z
dc.date.available2026-07-07T02:22:48Z
dc.descriptionWe 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.
dc.description4 pages, LaTeX, 4 figures (included). Accepted for publication in MNRAS
dc.identifierhttps://arxiv.org/abs/astro-ph/9701190
dc.identifierhttp://arxiv.org/abs/astro-ph/9701190
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11008
dc.subjectAstrophysics
dc.titleHigh-resolution radio observations of GX 339-4
dc.typetext

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