Sections Review
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Vocabulary
active galaxy | quasar | radio galaxy |
Seyfert galaxy |
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- Compare the luminosity and size of the power source for quasars to that of
a normal galaxy.
- Contrast the shape of the spectrum and the relative power at different
wavelength bands (X-ray, ultraviolet, visible, infrared, radio) for the energy
coming from quasars (and active galaxies) to that from mormal galaxies
(and stars).
- What produces the huge power output in quasars and active galaxies?
- What could cause the power generation to ``turn off'' and later turn back on?
- What determines the type of active galaxy (i.e., Seyfert 1 or 2, radio galaxy,
BL Lac, etc.) you will see?
- What is the broad-line emission region and what must the orientation of the
disk and dust ring be to see the broad-line emission region?
- What are the jets in active galaxies and how are they produced?
- Why are there many more quasars billions of light years away than nearby?
Include in your explanation a contrast of the conditions of the universe billions
of years ago to the current conditions.
- What does the changing number of quasars with increasing distances tell us about
the character of the universe?
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last updated: 26 May 2001
Is this page a copy of Strobel's
Astronomy Notes?
Author of original content:
Nick Strobel