Image Details
Caption: Fig. 10.
Same as Fig. 9, but for a run with full radiative transfer (C2; thick solid line), a run with self‐shielding above the physical density 10−2 cm−3 (C2s; thick dashed line), and a run with the optically thin approximation throughout the entire simulation volume (C2t; thick dotted line), all at ﹩z=3﹩.
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.