Fig. 6 from Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X‐Ray Luminosity Clusters

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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. 6.

Distribution of B/T ratios is shown for low‐density (lowest 5–25 percentile) and high‐density (highest 5–25 percentile) regions separately, as indicated. The low‐﹩L_{\mathrm{X}\,}﹩ cluster data are shown in the top panel, and the high‐﹩L_{\mathrm{X}\,}﹩ cluster data are shown in the bottom panel. Uncertainties are 1 σ and include the error in background subtraction.

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