Radio / X-ray correlation in the low/hard state of GX 339--4
arXiv:astro-ph/0301436 · doi:10.1051/0004-6361:20030090
Abstract
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.
8 pages. Accepted for publication in Astronomy & Astrophysics, 2003
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- Discovery of Jet-Induced Soft Lags of XTE J1550-564 during Its 1998 Outburst
- Galactic X-ray binary jets
- Correlations of Disk and Jet Emission Deviating from the Fundamental Plane
- Identifying Long Radio Transients with Accompanying X-Ray Emission as Disk-Jet Precessing Black Holes: The Case of ASKAP J1832-0911
- A magnetic model for low/hard state of black hole binaries
- The Galactic Black Holes Cyg X-1, GX 339-4, and 4U 1957+11: In Transition and at High Resolution
- Ultraviolet spectroscopy of the black hole X-ray binary MAXI J1820+070 across a state transition
- Accretion Geometry of Black Hole X-ray Binaries: Insights from X-ray Observations
- On the origin of core radio emissions from black hole sources in the realm of relativistic shocked accretion flow
- Probing the Jet Turnover Frequency Dependence on Black Hole Mass and Mass Accretion Rate
- Extreme Transients in Gamma Rays
- A multi-wavelength study of GRS 1716-249 in outburst : constraints on its system parameters
- The black hole X-ray binary MAXI J1348630 in quiescence
- A unified paradigm for the spectral and temporal evolution of Black Hole X-ray Binaries
- Neutrino flares from black hole coronae