Exam 13: Galaxies: Normal and Active
Exam 1: Here and Now97 Questions
Exam 2: A Users Guide to the Sky116 Questions
Exam 3: Cycles of the Sun and Moon154 Questions
Exam 4: The Origin of Modern Astronomy144 Questions
Exam 5: Light and Telescopes156 Questions
Exam 6: Atoms and Spectra125 Questions
Exam 7: The Sun146 Questions
Exam 8: The Family of Stars190 Questions
Exam 9: The Formation and Structure of Stars136 Questions
Exam 10: The Deaths of Stars127 Questions
Exam 11: Neutron Stars and Black Holes99 Questions
Exam 12: The Milky Way Galaxy117 Questions
Exam 13: Galaxies: Normal and Active151 Questions
Exam 14: Modern Cosmology112 Questions
Exam 15: The Origin of the Solar System108 Questions
Exam 16: Earth and Moon: Bases for Comparative Planetology98 Questions
Exam 17: Mercury, Venus, and Mars83 Questions
Exam 18: The Outer Solar System136 Questions
Exam 19: Meteorites, Asteroids, and Comets91 Questions
Exam 20: Astrobiology: Life on Other Worlds97 Questions
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In the double-exhaust model, the radio lobes of a radio galaxy are inflated by
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Which distance indicator technique is best to find distances to galaxies
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Centaurus A is a radio galaxy that has a visible galaxy at the center. This central elliptical galaxy of Centaurus A is encircled by a ring of gas and dust, different from most elliptical galaxies. The dust ring orbits about an axis that is perpendicular to the axis of rotation of the elliptical galaxy. What does this suggest about this central elliptical galaxy of Centaurus A
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-The red line shown above is shifted 15.8% from the blue dashed line. If Hβ is 486.1 nm, what is the change in the wavelength
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What evidence do we have that large galaxies cannibalize small galaxies
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___________ is (are) observed when light from a distant quasar travels past a massive galaxy between us and the quasar, and this light is focused to form two or more images of the same quasar.
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The hydrogen Balmer line Hβ has a wavelength of 486.1 nm in the laboratory. It is observed in a quasar at 2430.5 nm. What is the fractional change in wavelength or redshift z of this quasar
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When discovered in the 1960's, a(n) ___________ was found to emit large amounts of energy, but through visual and radio telescopes appeared to be a single point of light much like a star.
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The above visual wavelength image of a counter-clockwise rotating spiral galaxy indicates that the blueshifted emission lines are the dashed lines above the solid black horizontal line in the right panel and the redshifted emission lines are the dashed lines below the solid black horizontal line. 
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-The shells indicated in the enhanced visual wavelength image shown above are formed from _____________.
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Astronomers now speculate that a galaxy's shape depends on all of the following except
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If the absolute magnitude, M, of a supernova is −19 and a galaxy is found that contains a supernova with an apparent magnitude, m, of 16. What is the distance to the galaxy Hint: dpc =
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Discuss the observational differences between spiral, elliptical, and irregular galaxies.
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The figure shows an image of a galaxy at dust-penetrating wavelengths. It can be classified as which one of the following galactic types 
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Why are there few quasars at low redshifts and at high redshifts but many at redshifts of about 2
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Why do astronomers believe supermassive black holes are the source of an AGN's energy
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Which kind of active galaxies has been observed at the greatest distances from us
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Recent high resolution radio observations show that quasars can be classified as
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