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MOST Radio Monitoring of GX 339-4

D. C. Hannikainen, R. W. Hunstead, D. Campbell-Wilson, R. K. Sood

astro-pharXiv:astro-ph/9805332

Abstract

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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