Image Details
Caption: Fig. 4.
Distribution of internal reddening [E(B−V)int] for (a) all H II nuclei in our survey, (b) nuclei with types S0–Sbc, (c) nuclei with types Sc–I0, and (d) the sample of disk H II regions of McCall et al. (1985). The bins are separated by 0.1 mag. We estimated the internal reddening in our measurements from the observed Hα/Hβ ratio (see Ho et al. 1997a).
© 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.