HE0359-3959: an extremely radiating quasar
  We present a multiwavelength spectral study of the quasar HE0359-3959, which
has been identified as an extreme radiating source at intermediate redshift
(z=1.5209). Along the spectral range, the different ionic species give
information about the substructures in the broad line region. The presence of a
powerful outflow with an extreme blueshifted velocity of $\sim$-6000$\pm$500 km
s$^{-1}$ is shown in the CIV{\lambda}1549 emission line. A prominent
blueshifted component is also associated with the 1900{\AA} blend, resembling
the one observed in CIV{\lambda}1549. We detect a strong contribution of very
the low-ionization lines, FeII and Near-Infrared CaII triplet. We find that the
physical conditions for the low, intermediate and high-ionization emission
lines are different, which indicate that the emission lines are emitted in
different zones of the broad line region. The asymmetries shown by the profiles
reveal different forces over emitter zones. The high-ionization region is
strongly dominated by radiation forces, which also affect the low and
intermediate-ionization emitter region, commonly governed by virial motions.
These results support the idea that highly radiating sources host a slim disk.
