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Figure 1:
Top: B image of the dusty disk model
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Figure 2:
Behaviour of two-dimensional fits and residua for simulations done
in the B band, for
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Figure 3:
The ratio of the apparent to intrinsic scalelengths
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Figure 4:
The ratio of the apparent to intrinsic scalelengths
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Figure 5:
The ratio of the apparent to intrinsic scalelengths
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Figure 6:
The change in the ratio of the scalelengths in B and I bands due
to the effects of dust, plotted as
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Figure 7:
Comparison between the apparent ratios of scalelength in B and I predicted by our work (solid lines) and by the work of Cunow et al. (2001)
(dashed lines).
The curves are for
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Figure 8:
The ratio of the apparent average central surface brightness to
the intrinsic average central face-on surface brightness expressed in
magnitudes,
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Figure 9:
The ratio of the apparent average central surface brightness to
the intrinsic average central face-on surface brightness expressed in
magnitudes,
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Figure 10:
The ratio of the apparent average central surface brightness to
the intrinsic average central face-on surface brightness expressed in
magnitudes,
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Figure 11:
The change in the B-I central colour due to the effects of dust,
plotted as
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Figure 12:
The ratio of the apparent to intrinsic axis ratio
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Figure 13:
Observed scalelength ratios between B and I,
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