Tables 3 and 4 are only available in electronic form at http://www.edpsciences.org

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See Sect. 3.2 for the definition of inner disks.

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... hereafter RC3#

Inclination is derived from the axis ratio b/a, assuming an intrinsic disk thickness c/a = 0.2.

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... ratio

Erwin & Sparke (2003) found that the Ohta et al. measurements were a good match to their definition of $\ensuremath{L_{\rm bar}}$ , and the ellipse fits for this galaxy do not provide useful constraints.

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