: David L. Block, Kenneth C. Freeman, Ivânio Puerari
: David L. Block, Kenneth Freeman, Ivânio Puerari
: Galaxies and their Masks A Conference in Honour of K.C. Freeman, FRS
: Springer-Verlag
: 9781441973177
: 1
: CHF 190.00
:
: Astronomie
: English
: 479
: Wasserzeichen/DRM
: PC/MAC/eReader/Tablet
: PDF
Various kinds of masks obscure our view of our galaxy, the Milky Way, as well as of other galaxies. Masks of interstellar dust affect our measurements within galaxies, on scales ranging from individual supernovae to the galaxies themselves. The ,mass mask (our inability to image mass rather than light) gives astronomers a very incomplete picture of the size and structure of galaxies themselves, because we cannot image the dark matter which provides most of the galactic mass. Another mass is the dynamical mask: as galaxies form, much dynamical information is lost in the birthing process. A new thrust in research is to retrieve such information by means of chemical tagging. About 50 astronomers flew into Namibia in April 2010, to celebrate the 70th birthday of Professor K.C. Freeman, Fellow of the Royal Society. At age 70, Freeman, a father of dark matter in galaxies, continues to be one of planet's most highly cited astronomers. The current volume affords readers a unique perspective on galaxies by probing the thoughts of some of the greatest astronomers of our age. Contributions focus on galaxies from within our Local Group to those in our high redshift Universe. Approximately 40 in-depth review and contributed papers are contained in the volume, each written by an expert in the field. Two unusual features of the current volume include the Star Country of the San people of southern Africa as well as the introduction into astronomy of The Treachery of Images by the Belgian surrealist artist René Magritte. Everything we see hides another thing, we always want to see what is hidden by what we see, said Magritte. These words resonate the theme of the current volume Galaxies and their Masks, which is written at a level to be appreciated by both specialist and doctoral student alike.
Preface5
Contents15
A Tribute to Ken Freeman19
Stars are Small Dark-Coloured ThingsThat Live in Holes in the Ground 35
1 Introduction35
2 !nanni, Tamme and George Stow36
3 Concluding Thoughts53
References55
Shrouds of the Night -- Galaxies and René Magritte 57
1 Galaxies and René Magritte57
2 The Treachery of Conventional Images of Galaxies59
3 The Duality of Spiral Structure60
4 The Building of Galactic Disks: Active Evolutionin the Triangulum Spiral M3368
4.1 Farewell to Monolithic Collapse of M3370
5 Lessons from the Andromeda Spiral71
6 Conclusion -- ``La condition humaine''71
References74
Twin Masks of Spiral Structure? A Local Perspective 79
1 Introduction79
2 Approaches to Modeling80
3 Model Statistics and the Two-Arm / Four-Arm Dichotomy82
4 Central Bar90
References90
The Mask of Complexity in Disk Galaxies 93
1 Introduction93
2 Build-Up of Complication94
3 Modeling97
4 Toward Simplified Models of Disk Galaxies98
5 Conclusions99
References100
Cosmic Magnetic Fields -- An Overview 101
1 Introduction102
2 Observational Methods103
3 Magnetic Fields in the Milky Way105
4 Magnetic Fields in Galaxies110
5 More Distant Magnetic Fields115
6 Field Origin and Amplification115
References118
The Gaseous Halo Mask 121
1 Introduction121
2 Gas Stripping from Dwarf Galaxies122
3 Tracking the Evolution of Dwarf Galaxies in Cosmological Simulations124
4 What happens to the Stripped Gas?127
5 Summary129
References129
Molecular Gas Properties of Galaxies: The SMA CO(2-1) B0DEGA Legacy Project 131
1 Introduction131
2 The B0DEGA Sample132
3 Preliminary Results: CO(2--1) Morphologies and Concentration133
4 Discussion135
References137
The DiVA's Mask: Iconifying Galaxies and Revealing HI Anomalies 139
1 Introduction139
2 Observations, Analysis, and Modelling140
3 Preliminary Results142
3.1 Iconifying Galaxies142
3.2 Revealing HI Anomalies142
4 Summary and Future Plans145
References145
Enigmatic Masks of Cosmic Dust: Lessons from Nearby Galaxies Through the Eyes of the Spitzer Space Telescope 147
1 Introduction147
2 Two Form Families of Stellar-Barred Spirals at 8.0m148
2.1 Type 1: Tightly Coupled Morphologies at 3.6 and 8.0m149
2.2 Type 2: Straight and Curved Dust Lanes in Emission, Without Trace of a Bar150
3 Conclusion152
References153
The Large Magellanic Cloud: A Power Spectral Analysis of Spitzer Images 155
1 Introduction155
2 Data156
3 Analysis157
4 Results157
5 Simulations158
6 Conclusions161
References161
Light Cores Behind Dark Masks 163
1 Introduction163
2 Observations of NGC5236164
3 Modeling of NGC5236 Nucleus167
4 Observations of NGC253168
5 Concluding Remarks170
References170
Globalization, Open Access Publishing, and the Disappearance of Print: Threat or Opportunity? 173
1 Introduction173
2 Globalization174
3 Open Access Publishing176
4 The Disappearance of Print177
5 The Future178
References178
Super Star Clusters and Supernovae in Interacting LIRGs Unmasked by NIR Adaptive Optics 181
1 Introduction181
2 Super Star Cluster Candidates182
2.1 The SSC NIR Luminosity Function182
3 Searching for Extincted Core-Collapse SNe184
4 SF and Dynamics in Interacting Galaxies185
5 Summary186
References186
Structure, Mass, and Stability of Galactic Disks 187
1 Stellar Disks187
2 Stellar Kinematics188
3 Mass-to-Light Ratios and ``Maximum Disk''191
4 Flaring of HI Layers and Disk Masses193
5 Flatness and Truncations in Stellar Disks196
References200
What Can the Radial Surface Brightness Profiles of Galaxy Discs Tell Us About Their Evolution? 203
1 Profile Classifica