Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-01-22
Astron.Astrophys.400:1007-1012,2003
Astronomy and Astrophysics
Astrophysics
8 pages. Accepted for publication in Astronomy & Astrophysics, 2003
Scientific paper
10.1051/0004-6361:20030090
We present the results of a long-term study of the black hole candidate GX 339-4 using simultaneous radio (from the Australia Telescope Compact Array) and X-ray (from the Rossi X-ray Timing Explorer and BeppoSAX) observations performed between 1997 and 2000. We find strong evidence for a correlation between these two emission regimes that extends over more than three decades in X-ray flux, down to the quiescence level of GX 339-4. This is the strongest evidence to date for such strong coupling between radio and X-ray emission. We discuss these results in light of a jet model that can explain the radio/X-ray correlation. This could indicate that a significant fraction of the X-ray flux that is observed in the low-hard state of black hole candidates may be due to optically thin synchrotron emission from the compact jet.
Corbel Sephane
Fender Rob P.
Markoff Sera
Nowak Maciej A.
Tzioumis Anastasios K.
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