  Some of the most interesting types of astrophysical objects that have been
intensively studied in the recent years are the Anomalous X-ray Pulsars (AXPs)
and Soft Gamma-ray Repeaters (SGRs) seen usually as neutron stars pulsars with
super strong magnetic fields. However, in the last two years two SGRs with low
magnetic fields have been detected. Moreover, fast and very magnetic white
dwarf pulsars have also been observed in the last years. Based on these new
pulsar discoveries, white dwarf pulsars have been proposed as an alternative
explanation to the observational features of SGRs and AXPs. Here we present
several properties of these SGRs/AXPs as WD pulsar, in particular the surface
magnetic field and the magnetic dipole momentum.
