  Narrow Line Seyfert 1 galaxies are generally accreting at high fractions of
the Eddington limit. They can show complex X-ray spectra, with a strong `soft
excess' below 2 keV and a sharp drop at ~7 keV. There is strong evidence
linking the soft excess to either reflection or absorption from relativistic,
partially ionized material close to the black hole. The reflection models can
also simultaneously produce the 7 keV feature from fluorescent iron Ka line
emission from the disc. Here we show that absorption can also produce a sharp
feature at 7 keV from the P Cygni profile which results from
absorption/scattering/emission of He- and H-like iron Ka resonance lines in the
wind. We demonstrate this explicitly by fitting the iron feature seen in
XMM-Newton data from 1H 0707-495 to a P Cygni profile. The resulting column and
ionization required to produce this feature are probably larger than those
needed to produce the soft excess. Nonetheless, the absorbing material could
still be a single structure with stratified ionization such as that produced by
the ionization instability.
