Four quiescent elliptical galaxies were imaged with the NRAO VLA at 8.5 GHz
. Within the context of canonical advection-dominated accretion flows (ADAF
s), these VLA images plus published black hole masses constrain the accreti
on rates to be less than 1.6 x 10(-4), less than 3.6 x 10(-4), less than or
equal to 7.8 x 10(-4), and less than or equal to 7.4 x 10(-4) of the Eddin
gton rates. These ADAF accretion rates derived at 8.5 GHz have important im
plications for the levels of soft and hard X-rays expected from these quies
cent galaxies.