Exam 17: Active Galaxies and Supermassive Black Holes

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Head-tail galaxies are

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The hydrogen Balmer line H β\beta has a wavelength of 486.1 nm in the laboratory.It is observed in a quasar at 2430.5 nm.What is the red shift of this quasar?

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Most galaxies appear to be ...

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A(n)____ is observed if our line of sight is parallel to the plane of the dense disk of an active galactic nucleus.

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Why do astronomers believe black holes are the source of an AGN's energy?

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Some quasars have fuzz around them that produces spectra like that of normal galaxies.

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Radio lobes are held together by their magnetic fields.

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Encounters between galaxies would be ____ in the past versus now.

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How does the study of quasars reveal information of the history of the universe?

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In the unified model of active galactic nuclei,the broad line region in an active galactic nucleus is

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Astronomers can estimate the mass of the black hole at the center of the active galaxy M87 from the

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How are astronomers able to determine that quasars are so small?

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Astronomers who discovered quasars found that they show ________ of their spectral lines and are thus probably much ________ than nearby galaxies.

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If a quasar has a red shift of 0.98,then it is receding from the earth at 98 percent the speed of light.

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

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The disks which have been observed in the centers of some active galaxies evidently have a ____ at their centers.

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The hot gas of a radio lobe could be held together by

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Head-tail galaxies are pairs of galaxies interacting with each other.

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Double-lobed radio galaxies appear to be emitting jets of gas and radiation.

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We suspect that quasars are the active centers of galaxies because

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