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The stability of low surface brightness disks based on multi wavelength modeling

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Figure

Figure 1. High-resolution imaging of the inner regions (approximatelyshow the presence of dark clouds in their nuclear regions that are seen in lowernumbers in IC 2233
Table 2Intrinsic Stellar Template Model Parameters
Figure 4. Observed (left) and synthetic (right) images of UGC 7321 at, from top to bottom: B band, 3.6 μm, 8 μm, 70 μm, and 160 μm.(A color version of this figure is available in the online journal.)
Figure 6. Observed (left) and synthetic (right) images of NGC 4244 at, from top to bottom: r band, 3.6 μm band, 8 μm, 70 μm, and 160 μm.(A color version of this figure is available in the online journal.)
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