  A plasma made out of strange-quark matter (SQM) and electrons, has a rather
high plasma frequency (>20 MeV). Thus, a compact star made of such material all
the way up to its surface, i.e., a bare strange star, would be unable to
radiate away its thermal emission.
  We use the MIT-bag model and assume that SQM is the ground state of nuclear
matter at high density. We investigate whether the presence of a magnetic field
will allow propagation of radiation at frequencies below the SQM plasma
frequencies. Hence, we study the presence of gyrofrequencies in a SQM plasma
permeated by a strong magnetic field (B > 10^{12} G). We find that small
regions in the frequency spectrum allow radiation propagation due to the
presence of the magnetic fields. It is likely that narrow bands of radiation
would likely be observable from magnetized bare strange stars .
