  Many astrophysicists believe that Anomalous X-Ray Pulsars (AXP), Soft
Gamma-Ray Repeaters (SGR), Rotational Radio Transients (RRAT), Compact Central
Objects (CCO), and X-Ray Dim Isolated Neutron Stars (XDINS) belong to different
classes of anomalous objects with neutron stars as the central bodies inducing
all their observable peculiarities. We have shown earlier (I.F.Malov and
G.Z.Machabeli, Astron. Astrophys. Trans. 25, 7, 2006) that AXPs and SGRs could
be described by the drift model in the framework of preposition on usual
properties of the central neutron star (rotation periods P ~ 0.1 - 1 sec,
surface magnetic fields B ~ 10^11 - 10^13 G). Here we shall try to show that
some differences of considered sources will be explained by their geometry
(particularly, by the angle BETA between their rotation and magnetic axes). If
BETA < 10 deg. (the aligned rotator) the drift waves at the outer layers of the
neutron star magnetosphere should play a key role in the observable
periodicity. For large values of BETA (the case of the nearly orthogonal
rotator) an accretion from the surrounding medium (for example, from the relic
disk) can cause some modulation and transient events in received radiation.
