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Class introduction
Entire file in one
Postscript file
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Class introduction
Observational history
What are galaxies made of?
How are galaxies formed?
What limits the size of galaxies?
Observations of galaxies
Photometric
Spectroscopic
Morphological
Dark matter ``observations''
Measuring distances to galaxies
Galaxy catalogs and selection effects
Observable global properties of galaxies
Morphology-density relation
Galaxy luminosity function
Stellar populations
Chemical evolution models
Stellar populations and chemical evolution in nearby galaxies: the Local Group
Stellar populations in Local Group galaxies
Local Group formation
Elliptical galaxies
Stellar populations in ellipticals
Structure of ellipticals
Ellipticals: relation between global parameters and the fundamental plane
Dark matter in ellipticals
Spiral galaxies
Global relations for spirals: the Tully-Fisher relation
Stellar populations and star formation in spiral disks
Gas in spirals and correlation with SFR
Interaction of stars with the ISM
AGN
Bulges
Clusters and cluster galaxies
Observations of galaxies at higher redshift
Evolution of the luminosity function
Morphology of distant galaxies
Evolution of the luminosity density
Evolution of the stellar mass density
Evolution in clusters
High redshift galaxies
Absorption line systems
Galaxy formation models
Growth of perturbations in expanding universe for cold particles, within horizon
Distribution of overdensities in the Universe
Properties of halos
Properties of dark matter halos
Dissipation
Numerical models of galaxy formation
Jon Holtzman 2007-05-04
