  We clarify important physics issues related to the recently established new
mass limit for magnetized white dwarfs which is significantly
super-Chandrasekhar. The issues include, justification of high magnetic field
and the corresponding formation of stable white dwarfs, contribution of the
magnetic field to the total density and pressure, flux freezing, variation of
magnetic field and related currents therein. We also attempt to address the
observational connection of such highly magnetized white dwarfs.
