Spectroscopy of Outlying H II Regions in Spiral Galaxies: Abundances and Radial Gradients

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© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Liese van Zee et al 1998 AJ 116 2805 DOI 10.1086/300647

1538-3881/116/6/2805

Abstract

We present the results of low-dispersion optical spectroscopy of 186 H II regions spanning a range of radius in 13 spiral galaxies. Abundances for several elements (oxygen, nitrogen, neon, sulfur, and argon) were determined for 185 of the H II regions. As expected, low metallicities were found for the outlying H II regions of these spiral galaxies. Radial abundance gradients were derived for the 11 primary galaxies; similar to results for other spiral galaxies, the derived abundance gradients are typically -0.04 to -0.07 dex kpc-1.

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10.1086/300647