  We report on mid-infrared (MIR) continuum and line emission mapping of the
nucleus of NGC 253. The data, with a resolution of 1\as.4, reveal a
double-peaked arc-like [NeII] emission region. Comparison with published data
shows that the [NeII] arc is centered on the nucleus of the galaxy. The
brightest [NeII] source coincides with the infrared continuum peak. The
interpretation of these results is complicated by the edge-on orientation of
NGC 253, but a self-consistent explanation is starformation triggered by
dynamical resonances in a barred potential.
