Image Details
Caption: Fig. 10.
Comparison of angular momentum and density profiles. We show ﹩j^{2}/ rM\left(r\right)﹩ as a function of r for halo c (top) and halo d (middle) and ρ(r)r for halo d (bottom).
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.