Fig. 1 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. 1.

Eighteen galaxies (9 bright and 9 faint) randomly selected from the cluster and field samples. Apparent ﹩R_{702}﹩ magnitude and B/T values are shown in each panel. Each image is 6^{﹩\arcsec﹩} on a side and contours are arbitrarily spaced. The top row shows galaxies with ﹩B/ T< 0.1﹩, which are primarily spirals. Galaxies in the middle row have ﹩0.4< B/ T< 0.6﹩, while the bottom row shows galaxies with ﹩B/ T> 0.8﹩.

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