Image Details
Caption: Fig. 6.
Profiles of the Lyman absorption lines least contaminated by airglow emission and H2 absorption. Fluxes are in ergs cm−2 s−1 Å−1. Each line is identified by its rest wavelength and shifted vertically by ﹩2\times 10^{-14}﹩ to provide separation from the mean profile (thick solid line). Note the flat‐bottomed saturated absorption profiles and the large width in velocity.
© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.