  High resolution spectra of novae after outburst reveal distinctive
characteristics in the line profiles and intensities. The higher Balmer lines
are often broader than the lower members of the series, and the relative
profiles and intensities of the [O I] \lambda\lambda6300, 6364 doublet differ
from normal values. We suggest these features may be caused by the Quadratic
Zeeman Effect from magnetic fields exceeding B=10^6 gauss. Taken together the
emission and absorption lines point to multiple origins for the ejecta on both
the erupting white dwarf and the cool secondary star.
