Fig. 7 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. 7.

B/T distribution for galaxies with ﹩\Sigma _{\mathrm{local}\,}=50﹩–200 ﹩h^{2}_{50}﹩ Mpc﹩^{-2}﹩. The solid and dotted histograms correspond to the low‐﹩L_{\mathrm{X}\,}﹩ and high‐﹩L_{\mathrm{X}\,}﹩ samples, respectively.

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