  We discuss the options of the fall-back disk model of Anomalous X-Ray Pulsars
(AXPs). We argue that the power-law index of the mass inflow rate during the
propeller stage can be lower than those employed in earlier models. We take
into account the effect of the super-critical mass inflow at the earliest
stages on the inner radius of the disk and argue that the system starts as a
propeller. Our results show that, assuming a fraction of the mass inflow is
accreted onto the neutron star, the fall-back disk scenario can produce AXPs
for acceptable parameters.
