Exam 13: Galaxies: Normal and Active

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___________ have elongated nuclei with spiral structure extending from the ends of the elongations. The Milky Way is a member of this class of galaxy.

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We should expect galaxies to collide fairly often because

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The energy from an AGN is produced by

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That the radio lobes radiate synchrotron radiation indicates that

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What factors are important when trying to classify a spiral galaxy

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What observational evidence do we have that quasars are the centers of very distant galaxies

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____________ galaxies contain a supermassive black hole at their centers while active nuclei are present in ____________of galaxies

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Most galaxies appear to be

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How are astronomers able to determine that quasars are so small

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The rotation curve method can be applied only to pairs of galaxies orbiting each other.

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The blue sharp point of light with diffraction spikes in the upper right corner of the visual + NIR image of the Hubble Deep Field, shown above, is a star in our Milky Way Galaxy. The blue sharp point of light with diffraction spikes in the upper right corner of the visual + NIR image of the Hubble Deep Field, shown above, is a star in our Milky Way Galaxy.

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Most of the mass of a galaxy is contained in the

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Jet-shaped regions of radio and optical emission have been observed in

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in the following visual wavelength image, the two galaxies shown are most likely to have formed from ____________. in the following visual wavelength image, the two galaxies shown are most likely to have formed from ____________.

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What is the major observational difference between a Seyfert galaxy and a normal spiral galaxy

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________________ emit radio energy from areas on either side of the galaxy that are inflated by jets.

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According to the unified model of active galactic nuclei, ___________ is in the center surrounded by _____________with a Type 1 Seyfert or Type 2 Seyfert being seen depending on the viewing angle.

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Describe the kind of observations that have led astronomers to believe that supermassive black holes lie at the center of many galaxies.

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The above visual wavelength image shows galaxies interacting. The above visual wavelength image shows galaxies interacting.

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What distance method did Edwin Hubble use to determine the distance to local galaxies

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