  In previous work we found that the spectral state switch and other spectral
properties of both neutron star (NS) and galactic black hole candidates (GBHC),
in low mass x-ray binary systems could be explained by a magnetic propeller
effect that requires an intrinsically magnetic central compact object. In later
work we showed that intrinsically magnetic GBHC could be easily accommodated by
general relativity in terms of magnetospheric eternally collapsing objects
(MECO), with lifetimes greater than a Hubble time, and examined some of their
spectral properties. In this work we show how a standard thin accretion disk
and corona can interact with the central magnetic field in atoll class NS, and
GBHC and active galactic nuclei (AGN) modeled as MECO, to produce jets that
emit radio through infrared luminosity $L_R$ that is correlated with mass and
x-ray luminosity as $L_R \propto M^{0.75 - 0.92}L_x^{2/3}$ up to a mass scale
invariant cutoff at the low/high spectral state switch. Comparing the
MECO-GBHC/AGN model to observations, we find that the correlation exponent, the
mass scale invariant cutoff, and the radio luminosity ratios of AGN, GBHC and
atoll class NS are correctly predicted, which strongly implies that GBHC and
AGN have observable intrinsic magnetic moments and hence do not have event
horizons.
