We present the results of low-dispersion optical spectroscopy of 186 H II r
egions spanning a range of radius in 13 spiral galaxies. Abundances for sev
eral elements (oxygen, nitrogen, neon, sulfur, and argon) were determined f
or 185 of the H II regions. As expected, low metallicities were found for t
he outlying H II regions of these spiral galaxies. Radial abundance gradien
ts were derived for the II primary galaxies; similar to results for other s
piral galaxies, the derived abundance gradients are typically -0.04 to -0.0
7 dex kpc(-1).