1
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- 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
- The Nuclear Bulge
- The Rotation curve and the Galaxy’s mass
- The origin of the galaxy
- The Galactic Center
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2
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- Family of Galaxies
- Properties of Galaxies
- Distance; The Hubble Law
- Size and Luminosity
- Mass (including Dark Matter)
- Evolution of Galaxies
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3
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- 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
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4
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- 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
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5
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- 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.
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6
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- 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.
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