Image Details
Caption: Fig. 4.
Spectral regions used to measure the H I column density. The upper panel shows the Lyα line, with the core and damping wing regions used in the fit shaded gray. The lower panel shows the absorption near the Lyman limit. Overlayed is the single‐component fit to the hydrogen with a column density of ﹩\mathrm{log}\,N_{\mathrm{H}\,\,{}^{{\rm{\small I}}}}=19.422﹩ cm−2 from Table 2.
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.