Image Details
Caption: Fig. 4.
Emission‐line flux as a function of position along the slit as measured in the UVES spectra with 1﹩\arcsec﹩‐wide extractions. The spatial profiles are normalized such that the area under each curve is equal, with the exception of [S II] λ6716, which is scaled to the same normalization as [S II] λ6731.
© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.