MOST Radio Monitoring of GX 339-4

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.

arXiv comment5 pages, 4 figures. Accepted for publication in Astronomy and Astrophysics

Cited by in corpus (4)

• The INTEGRAL view on Black Hole X-ray Binaries
• From Multiwavelength to Mass Scaling: Accretion and Ejection in Microquasars and AGN
• Accretion-ejection in rotating black holes: a model for `outliers' track of radio-X-ray correlation in X-ray binaries
• The Galactic Black Holes Cyg X-1, GX 339-4, and 4U 1957+11: In Transition and at High Resolution