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arxiv: astro-ph/9805332 · v1 · submitted 1998-05-27 · 🌌 astro-ph

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MOST Radio Monitoring of GX 339-4

D.C. Hannikainen , R.W. Hunstead , D. Campbell-Wilson , R.K. Sood
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classification 🌌 astro-ph
keywords monitoringradioaprilbeenbinaryblackcandidatecorrelation
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The Molonglo Observatory Synthesis Telescope (MOST) has been monitoring the candidate Galactic black hole binary system GX 339-4 at 843 MHz since 1994 April. We present the results of this program up to 1997 February and show a possible correlation between radio and X-ray light curves.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Multi-wavelength outburst activity from EP J174942.2-384834: a very faint X-ray transient discovered by Einstein Probe

    astro-ph.HE 2026-05 accept novelty 5.0

    EP J174942.2-384834 is classified as a very faint X-ray transient black hole candidate based on its hard X-ray spectra, optical/UV brightening correlated with X-rays, and lack of radio emission.