  The dichotomy between radio-loud and radio-quiet QSOs is not simply one of
host morphology. While spiral galaxies almost exclusively host radio-quiet
QSOs, ellipticals can host either radio-louds or radio-quiets. We find that a
combination of accretion rate and host scale determines which type of QSO a
given elliptical galaxy will host. QSOs with high x-ray luminosities (above
10^44.5 erg/s at 0.5 keV) are mostly radio-loud. But those with low
luminosities divide fairly neatly in size (measured by the half-light radius,
r_e). Those larger than about 10 kpc are radio-loud, while smaller ones are
radio-quiet. It has recently been found that core and coreless ellipticals are
also divided near this limit. This implies that for low-luminosity QSOs,
radio-louds are found in core ellipticals, while radio-quiets are in coreless
ellipticals and spirals. This segregation also shows up strongly for
low-redshift objects, and in general, there is a loss over time of coreless,
radio-loud QSOs. Since the presence or absence of a core may be tied to the
galactic merger history, we have an evolutionary explanation for the
differences between radio-loud and radio-quiet QSOs.
