Radio precedes X-ray Compton luminosity by ~3 days in the rising hard state but lags by ~8 days in the decaying hard state of GX 339-4, with inner magnetic field strength estimated from accretion rate and truncation radius accounting for both.
Nature627(8005):763–766
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A synthesis of multi-wavelength observations and models of variability, jets, and polarization in stellar-mass black hole accretion systems.
citing papers explorer
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Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion
Radio precedes X-ray Compton luminosity by ~3 days in the rising hard state but lags by ~8 days in the decaying hard state of GX 339-4, with inner magnetic field strength estimated from accretion rate and truncation radius accounting for both.
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Accreting stellar-mass black holes
A synthesis of multi-wavelength observations and models of variability, jets, and polarization in stellar-mass black hole accretion systems.