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On the Radial Density Profile of Intracluster Gas Tracing the Isothermal Dark Halo with a Finite Core
Wu & Xue 2000 The Astrophysical Journal 542 578.
Caption: Fig. 5.
Same as Fig. 4, but for NFW profile and β model. The dotted line shows the best‐fit relation excluding A119, A1367, A1656, and A2255.
© 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.