Notes
Slide Show
Outline
1
Review Chapter 12: Milky Way
    • The discovery of the Galaxy
      • Variable stars as distance indicators
      • Globular clusters
    • The size and overall structure of the Galaxy
    • 21 cm Hydrogen emission
    • Motions in the galaxy
      • The Halo
      • The Disk population
        • Spiral Arms
      • The Nuclear Bulge
      • The Rotation curve and the Galaxy’s mass
    • The origin of the galaxy
    • The Galactic Center
2
Chapter 13: Galaxies
  • Family of Galaxies
    • Classification
  • Properties of Galaxies
    • Distance; The Hubble Law
    • Size and Luminosity
    • Mass (including Dark Matter)
  • Evolution of Galaxies
    • Clusters
    • Mergers
3
Chapter 14: Galaxies with Active Nuclei
  • Discovery of Active Galactic Nuclei (AGN)
    • Seyfert Galaxies and Radio Sources
  • The Unified Model
    • Black Holes in Galaxies, disks, orientation, +
  • Quasars
    • Distances and Relativistic Redshifts
    • Quasars as extreme AGN
    • Evolution of Quasars/Galaxies
    • Gravitational Lensing
4
Chapter 15: Cosmology
  • The Hubble Expansion – review+
  • Olber’s paradox
  • The Big Bang
  • Refining the Big Bang
  • Details of the Big Bang
  • General Relativity
  • Cosmological Constant
  • Origin of Structure


5
Exam #3 on Mon., April 19
  • Sample questions.



    • The assumption of Isotropy states that
      • A. The universe looks the same at all epochs.
      • B. The universe looks the same from all locations over large enough distances.
      • C. The universe looks the same in all locations over large enough distances.
      • D. All of the above.
      • E. None of the above.

6
Exam #3 on Mon., April 19
  • Sample questions.
    • In order to determine the age of the universe, we require
      • A. The universe to be flat.
      • B. The amount of dark matter to be determined.
      • C. The redshifts of galaxies in the Local Group to be measured.
      • D. An accuration temperature of the background radiation.
      • E. The Hubble Constant and the density of the universe to be determined.

    • The center of our galaxy lies in the direction of the constellation of
      • A. Ursa Minor.
      • B. Ursa Major.
      • C. Sagittarius.
      • D. Orion.
      • E. Andromeda.