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Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X‐Ray Luminosity Clusters

  • Authors: Michael L. Balogh, Ian Smail, R. G. Bower, B. L. Ziegler, G. P. Smith, Roger L. Davies, A. Gaztelu, J.-P. Kneib, and H. Ebeling

Balogh et al. 2002 The Astrophysical Journal 566 123.

  • Provider: AAS Journals

Caption: Fig. 3.

Left: The distribution of B/T in the eight low‐﹩L_{\mathrm{X}\,}﹩ clusters and the mean distribution of the MDS field sample. For the eight clusters, the dotted histograms show the distribution of all galaxies, and the solid histograms are corrected for foreground and background contamination by subtracting the field distribution. Right: The B/T distributions of the high‐﹩L_{\mathrm{X}\,}﹩ clusters.

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