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Astron. Astrophys. 337, 460-464 (1998)


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MOST radio monitoring of GX 339-4

D.C. Hannikainen 1, R.W. Hunstead 2, D. Campbell-Wilson 2 and R.K. Sood 3

1 Observatory, P.O. Box 14, 00014 University of Helsinki, Finland (diana@carina.astro.helsinki.fi)
2 School of Physics, University of Sydney, NSW 2006, Australia
3 School of Physics, Australian Defence Force Academy, Canberra, ACT 2600, Australia

Received 27 April 1998 / Accepted 12 June 1998

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.

Key words: binaries – stars: individual: GX 339 – 4

Send offprint requests to: D.C. Hannikainen

© European Southern Observatory (ESO) 1998

Online publication: August 17, 1998

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