  This paper reports on the spectroscopic investigation of 101 Cepheids in the
Carina region. These Cepheids extend previous samples by about 35% in number
and increase the amount of the galactic disk coverage especially in the
direction of l \approx 270{\deg}. The new Cepheids do not add much information
to the radial gradient, but provide a substantial increase in azimuthal
coverage. We find no azimuthal dependence in abundance over an 80{\deg} angle
from the galactic center in an annulus of 1 kpc depth centered on the Sun. A
simple linear fit to the Cepheid data yields a gradient d[Fe/H]/dRG = -0.055
\pm 0.003 dex/kpc which is somewhat shallower than found from our previous,
smaller Cepheid sample.
