Image Details
Caption: Fig. 3.
Histogram of the number of Chandra sources detected above a certain ﹩L_{\mathrm{X}\,}﹩ [﹩N( > L_{\mathrm{X}\,}) ﹩] vs. ﹩L_{\mathrm{X}\,}﹩ [0.5–2.5 keV] for four globular clusters.
© 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.