Image Details
Caption: Fig. 2.
Distribution of NIC2 semimajor axis effective radius ﹩r_{e}﹩ from the GIM2D pure de Vaucouleurs bulge fits to our high‐redshift BCG sample (black histogram) compared to the local Abell sample of Graham et al. (1996; shaded histogram).
© 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.