| Preface | 5 |
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| Contents | 15 |
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| A Tribute to Ken Freeman | 19 |
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| Stars are Small Dark-Coloured ThingsThat Live in Holes in the Ground | 35 |
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| 1 Introduction | 35 |
| 2 !nanni, Tamme and George Stow | 36 |
| 3 Concluding Thoughts | 53 |
| References | 55 |
| Shrouds of the Night -- Galaxies and René Magritte | 57 |
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| 1 Galaxies and René Magritte | 57 |
| 2 The Treachery of Conventional Images of Galaxies | 59 |
| 3 The Duality of Spiral Structure | 60 |
| 4 The Building of Galactic Disks: Active Evolutionin the Triangulum Spiral M33 | 68 |
| 4.1 Farewell to Monolithic Collapse of M33 | 70 |
| 5 Lessons from the Andromeda Spiral | 71 |
| 6 Conclusion -- ``La condition humaine'' | 71 |
| References | 74 |
| Twin Masks of Spiral Structure? A Local Perspective | 79 |
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| 1 Introduction | 79 |
| 2 Approaches to Modeling | 80 |
| 3 Model Statistics and the Two-Arm / Four-Arm Dichotomy | 82 |
| 4 Central Bar | 90 |
| References | 90 |
| The Mask of Complexity in Disk Galaxies | 93 |
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| 1 Introduction | 93 |
| 2 Build-Up of Complication | 94 |
| 3 Modeling | 97 |
| 4 Toward Simplified Models of Disk Galaxies | 98 |
| 5 Conclusions | 99 |
| References | 100 |
| Cosmic Magnetic Fields -- An Overview | 101 |
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| 1 Introduction | 102 |
| 2 Observational Methods | 103 |
| 3 Magnetic Fields in the Milky Way | 105 |
| 4 Magnetic Fields in Galaxies | 110 |
| 5 More Distant Magnetic Fields | 115 |
| 6 Field Origin and Amplification | 115 |
| References | 118 |
| The Gaseous Halo Mask | 121 |
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| 1 Introduction | 121 |
| 2 Gas Stripping from Dwarf Galaxies | 122 |
| 3 Tracking the Evolution of Dwarf Galaxies in Cosmological Simulations | 124 |
| 4 What happens to the Stripped Gas? | 127 |
| 5 Summary | 129 |
| References | 129 |
| Molecular Gas Properties of Galaxies: The SMA CO(2-1) B0DEGA Legacy Project | 131 |
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| 1 Introduction | 131 |
| 2 The B0DEGA Sample | 132 |
| 3 Preliminary Results: CO(2--1) Morphologies and Concentration | 133 |
| 4 Discussion | 135 |
| References | 137 |
| The DiVA's Mask: Iconifying Galaxies and Revealing HI Anomalies | 139 |
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| 1 Introduction | 139 |
| 2 Observations, Analysis, and Modelling | 140 |
| 3 Preliminary Results | 142 |
| 3.1 Iconifying Galaxies | 142 |
| 3.2 Revealing HI Anomalies | 142 |
| 4 Summary and Future Plans | 145 |
| References | 145 |
| Enigmatic Masks of Cosmic Dust: Lessons from Nearby Galaxies Through the Eyes of the Spitzer Space Telescope | 147 |
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| 1 Introduction | 147 |
| 2 Two Form Families of Stellar-Barred Spirals at 8.0m | 148 |
| 2.1 Type 1: Tightly Coupled Morphologies at 3.6 and 8.0m | 149 |
| 2.2 Type 2: Straight and Curved Dust Lanes in Emission, Without Trace of a Bar | 150 |
| 3 Conclusion | 152 |
| References | 153 |
| The Large Magellanic Cloud: A Power Spectral Analysis of Spitzer Images | 155 |
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| 1 Introduction | 155 |
| 2 Data | 156 |
| 3 Analysis | 157 |
| 4 Results | 157 |
| 5 Simulations | 158 |
| 6 Conclusions | 161 |
| References | 161 |
| Light Cores Behind Dark Masks | 163 |
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| 1 Introduction | 163 |
| 2 Observations of NGC5236 | 164 |
| 3 Modeling of NGC5236 Nucleus | 167 |
| 4 Observations of NGC253 | 168 |
| 5 Concluding Remarks | 170 |
| References | 170 |
| Globalization, Open Access Publishing, and the Disappearance of Print: Threat or Opportunity? | 173 |
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| 1 Introduction | 173 |
| 2 Globalization | 174 |
| 3 Open Access Publishing | 176 |
| 4 The Disappearance of Print | 177 |
| 5 The Future | 178 |
| References | 178 |
| Super Star Clusters and Supernovae in Interacting LIRGs Unmasked by NIR Adaptive Optics | 181 |
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| 1 Introduction | 181 |
| 2 Super Star Cluster Candidates | 182 |
| 2.1 The SSC NIR Luminosity Function | 182 |
| 3 Searching for Extincted Core-Collapse SNe | 184 |
| 4 SF and Dynamics in Interacting Galaxies | 185 |
| 5 Summary | 186 |
| References | 186 |
| Structure, Mass, and Stability of Galactic Disks | 187 |
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| 1 Stellar Disks | 187 |
| 2 Stellar Kinematics | 188 |
| 3 Mass-to-Light Ratios and ``Maximum Disk'' | 191 |
| 4 Flaring of HI Layers and Disk Masses | 193 |
| 5 Flatness and Truncations in Stellar Disks | 196 |
| References | 200 |
| What Can the Radial Surface Brightness Profiles of Galaxy Discs Tell Us About Their Evolution? | 203 |
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| 1 Profile Classifica
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