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: http://zebu.uoregon.edu/tandf/toc.html
Дата изменения: Fri Jul 17 06:47:39 1998 Дата индексирования: Mon Oct 1 21:21:37 2012 Кодировка: Поисковые слова: coma |
1.1.1 Ancestors of our Modern Cosmological Model
1.1.2 The Legacy of the Ancient Greeks
1.1.3 Towards Renaissance Cosmology
1.1.4 Towards the Physical Universe
1.1.5 How Far to the Nearest Star?
1.1.6 General and Special Relativity
1.1.7 Einsteins Biggest Blunder?
1.1.8 The Discovery of Universal Expansion
1.1.9 Models of a Dense Universe
1.1.10 The Discovery of the Cosmic Microwave Background
1.1.11 The Hot Big Bang Model
1.2.1 The Robertson-Walker Metric
1.2.2 The Dynamics of an Expanding Universe
1.30 Modern Cosmological Puzzles
2.2 Possible Kinds of Cosmological Models
2.3 Establishing the Extragalactic Distance Scale
2.3.1 The First Rung: Calibrating the Main Sequence Luminosities of Stars
via Stellar Parallax
2.3.2 The Second Rung: Distances to stellar clusters
2.3.3 The Third Rung: Determining the Zeropoints of Standard Candles
2.3.4 Distances to Local Group Galaxies
2.3.5 Extragalactic Distance Indicators
2.3.6 The Distance to the Virgo Cluster
2.3.7 Correction for Bias in Extragalactic Samples
2.3.8 Hubble Space Telescope Distance Estimates to Virgo
2.3.9 Summary of Virgo Distance Estimates
2.3.10 Direct Astrophysical Distance Measurements
3.2.1 Groups of Galaxies
3.2.2 Clusters of Galaxies
3.2.3 Clusters of clusters: Superclusters
3.4 There's More Out There Than Just Light
3.5 Redshift Surveys: Defining Physical Structures
3.5.1 Hierarchical Clustering Patterns
3.5.2 The Coming of the Stickman
3.5.3 The Void in Bootes
3.5.4 The Deeply Probed Universe
3.5.5 Correlation Scales
3.6 The Peculiar Velocity Field
3.6.1 Inflows and Outflows
3.6.2 Virgocentric Flow
3.6.3 Large Scale Flows: Continental Drift in the Nearby Universe?
3.6.4 Infall Around the Great Attractor: A Case Study
3.7 The Physical Structure of Voids and Walls: A Case Study
3.8 A Really, Really Big Flow?
3.9 A Determination of Ho Using the Virgo and Coma Clusters
4.2.1 The Solar System
4.2.2 The Solar Neighborhood
4.2.3 Galactic Scales
4.3 Other Dark Matter Indicators for Galaxies
4.3.1 Hot Halos Around Elliptical Galaxies
4.3.2 Binary Galaxies
4.3.3 Stellar Population Effects on Mass-to-Light Ratios
4.3.4 Some Measured Values for M/L
4.3.5 Clusters of Galaxies
4.5 The Inflationary Paradigm and OMEGA = 1
4.6 Dark Matter Candidates and Detection
4.7 Further Implications of Dark Matter
4.8 Summary
5.2 Statistical Characterization of Structure
5.2.1 What Comes First - Galaxy-size or Cluster-size Potentials?
5.2.2 Biasing in the Universe
5.3.1 The Power Spectrum of the Galaxy Distribution
5.3.2 Can CDM be Saved?
5.3.3 Beyond CDM: More Exotic Scenarios
5.4 Observational Constraints
5.4.2 Small Scale Constraints
5.4.1 Large Scale Constraints
5.5 Summary
6.1.6 A Possible Decaying Particle Background
6.2.1 The Luminosity Function of Galaxies
6.2.2 Deep Galaxy Counts: The Mystery of the Faint Blue Galaxies
6.2.3 A New Population of Galaxies at z =0
6.3 Surface Brightness Selection Effects
6.3.1 Diameter Limited catalogs
6.3.2 Flux Limited Catalogs
6.4 Discovering Low Surface Brightness Galaxies
6.4.1 The Space Density of Galaxies as a Function of surface brightness
6.4.2 The Properties of LSB Galaxies
6.5.3 Cosmological Relevance of LSB Galaxies
6.5 Summary
7.3 Future Observations