Jr. Herrnstein et al., VLBA CONTINUUM OBSERVATIONS OF NGC-4258 - CONSTRAINTS ON AN ADVECTION-DOMINATED ACCRETION FLOW, The Astrophysical journal, 497(2), 1998, pp. 69-73
We report a 3 sigma upper limit of 220 mu Jy on any 22 GHz continuum e
mission coincident with the central engine in NGC 4258. If NGC 4258 is
powered by an advection-dominated accretion flow, this radio upper li
mit implies that the inner advection-dominated flow cannot extend sign
ificantly beyond similar to 10(2) Schwarzschild radii.