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Einführung in die Astronomie II
World Models
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  • Introduction to Astronomy I
  • Introduction to Astronomy II
    • Preamble
    • Introduction
    • Supernovae \& Gamma Ray Bursts
    • Galaxies: Classification
    • The Milky Way and the Galactic Center
    • Morphology of the Galaxy
    • Galaxies: Dynamics \& Masses
    • The Astronomical Distance Ladder
    • Active Galactic Nuclei
    • Clusters of Galaxies
    • World Models
    • The Big Bang
    • Determination of Omega
    • Determination of Lambda
    • Evolution of the Universe
Introduction
Introduction
Expansion of the Universe
Redshifts, Hubble Relation, Homogeneity, Isotropy, World Models, Friedmann Equations, Hubble's Law
World Models
Critical Density
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Introduction: IntroductionExpansion of the Universe: RedshiftsExpansion of the Universe: RedshiftsExpansion of the Universe: Hubble Relation
Expansion of the Universe: Hubble RelationExpansion of the Universe: HomogeneityExpansion of the Universe: HomogeneityExpansion of the Universe: Isotropy
Expansion of the Universe: World ModelsExpansion of the Universe: World ModelsExpansion of the Universe: Friedmann EquationsExpansion of the Universe: Friedmann Equations
Expansion of the Universe: Friedmann EquationsExpansion of the Universe: Friedmann EquationsExpansion of the Universe: Hubble's LawExpansion of the Universe: Hubble's Law
World Models: Critical DensityWorld Models: Critical DensityWorld Models: Critical DensityWorld Models: Critical Density
World Models: Critical Density  
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Jörn Wilms / joern.wilms@sternwarte.uni-erlangen.de