Exam 16: Normal and Active Galaxies: Building Blocks of the Universe
Exam 1: Charting the Heavens: the Foundations of Astronomy108 Questions
Exam 2: The Copernican Revolution: the Birth of Modern Science68 Questions
Exam 3: Light and Matter: the Inner Workings of the Cosmos112 Questions
Exam 4: Telescopes: the Tools of Astronomy99 Questions
Exam 5: The Solar System: Interplanetary Matter and the Birth of the Planets148 Questions
Exam 6: Earth and Its Moon: Our Cosmic Backyard149 Questions
Exam 7: The Terrestrial Planets: a Study in Contrasts132 Questions
Exam 8: The Jovian Planets: Giants of the Solar System123 Questions
Exam 9: Moons, Rings, and Plutoids: Small Worlds Among Giants161 Questions
Exam 10: The Sun: Our Parent Star124 Questions
Exam 11: Measuring the Stars: Giants, Dwarfs, and the Main Sequence154 Questions
Exam 12: The Interstellar Medium: Star Formation in the Milky Way128 Questions
Exam 13: Stellar Evolution: the Lives and Deaths of Stars167 Questions
Exam 14: Neutron Stars and Black Holes: Strange States of Matter131 Questions
Exam 15: The Milky Way Galaxy: a Spiral in Space166 Questions
Exam 16: Normal and Active Galaxies: Building Blocks of the Universe175 Questions
Exam 17: Hubbles Law and Dark Matter: the Large-Scale Structure of the Cosmos119 Questions
Exam 18: Cosmology: the Big Bang and the Fate of the Universe150 Questions
Exam 19: Life in the Universe: Are We Alone114 Questions
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A property common to active galaxies is that their energy is primarily .
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Our own Milky Way's Hubble class, according to the best data, is
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Synchrotron radiation is the major source of energy for active galaxies.
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A Type Sa galaxy is a spiral with a large bulge and tightly wound arms.
(True/False)
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The Tully- Fisher relation uses the rotational speed of the galaxy to measure its .
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Quasars are far enough away that we must take the relativistic redshift into account when calculating their age.
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According to Hubble's Law, the greater a galaxy's redshift, the
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Why is the energy source for active nuclei like Seyferts thought to be compact?
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The spectrum of radio galaxies indicates the energy is in radiation.
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Nearby active galaxies, such as Centaurus A, are likely the mergers between colliding galaxies.
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How does the light from active galaxies differ from that of a normal galaxy?
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As with our own Sun among the neighboring stars, most galaxies in the Local Group are smaller and dimmer than our own Milky Way.
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The elliptical galaxies have compositions and shapes like the _ of the Milky Way.
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