  This paper reports on the spectroscopic investigation of 238 Cepheids in the
northern sky. Of these stars, about 150 are new to the study of the galactic
abundance gradient. These new Cepheids bring the total number of Cepheids
involved in abundance distribution studies to over 400. In this work we also
consider systematics between various studies and also those which result from
the choice of models. We find systematic variations exist at the 0.06 dex level
both between studies and model atmospheres. In order to control the systematic
effects our final gradients depend only on abundances derived herein. A simple
linear fit to the Cepheid data from 398 stars yields a gradient d[Fe/H]/dRG =
-0.062 \pm 0.002 dex/kpc which is in good agreement with previously determined
values. We have also reexamined the region of the "metallicity island" of Luck
et al. (2006). With the doubling of the sample in that region and our
internally consistent abundances, we find there is scant evidence for a
distinct island. We also find in our sample the first reported Cepheid (V1033
Cyg) with a pronounced Li feature. The Li abundance is consistent with the star
being on its red-ward pass towards the first giant branch.
