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Multiple Choice
A) galaxies appear to be moving away from us.
B) their light comes predominantly from objects other than stars.
C) most galaxies contain clouds of gas that are absorbing their favorite wavelengths.
D) galaxies in the past rotated at a faster rate than they do today.
E) galaxies are rushing through space in all directions.
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Multiple Choice
A) They measured the velocities of stars in the inner regions of the galaxies.
B) They measured the rotation rates of gas as a function of distance from the centers of the galaxies.
C) They measured the amount of gravitational pull elliptical galaxies have on companion galaxies.
D) They assumed that the proportion of dark matter was roughly the same as in spiral galaxies.
E) They measured the X-ray emission from hot gas gravitationally bound to the galaxies.
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Multiple Choice
A) elementary particles that have mass but do not interact much with normal matter.
B) supermassive black holes.
C) faint stellar remnants such as white dwarfs and neutron stars.
D) free-floating Jupiter-mass planets.
E) cold concentrations of dust.
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Multiple Choice
A) a giant elliptical
B) an ordinary spiral galaxy
C) an irregular galaxy
D) a barred spiral
E) a dwarf elliptical
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Multiple Choice
A) UV.
B) X-rays.
C) gamma rays.
D) infrared.
E) radio.
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Multiple Choice
A) it absorbs only some wavelengths of light but not all wavelengths as dark matter does.
B) it interacts with light.
C) it is found only in spiral disks, whereas dark matter is also found in elliptical galaxies.
D) dust is easily destroyed by dark matter.
E) there is never enough to account for all the gravity in galaxies.
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Multiple Choice
A) there were fewer galaxy-galaxy interactions in the past.
B) there were more galaxy-galaxy interactions in the past.
C) supermassive black holes were larger in the past.
D) today's AGNs are hidden primarily by large amounts of cold gas and dust.
E) AGNs had bigger central black holes in the past.
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Multiple Choice
A) color and redshift.
B) star formation rate and morphological type.
C) width of emission lines and black hole accretion rate.
D) rotational speed and luminosity.
E) dark matter radial profile and X-ray brightness.
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Multiple Choice
A) 220 Mpc.
B) 450 Mpc.
C) 100 Mpc.
D) 15,400 Mpc.
E) 100 kpc.
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Multiple Choice
A) 695.7 nm
B) 719.4 nm
C) 742.3 nm
D) 765.7 nm
E) 1,750 nm
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Multiple Choice
A) 0.05
B) 0.07
C) 0.10
D) 0.13
E) 0.15
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Essay
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Essay
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Multiple Choice
A) 1,083 nm
B) 1,183 nm
C) 1,248 nm
D) 1,440 nm
E) 3,142 nm
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Multiple Choice
A) 0.3 Mpc
B) 40 Mpc
C) 1,200 Mpc
D) 1,800 Mpc
E) 3,500 Mpc
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Essay
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Multiple Choice
A) X-ray
B) gamma-ray
C) radio
D) infrared
E) visible
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Essay
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Multiple Choice
A) tightness of the spiral arms.
B) luminosity of the galaxy.
C) age of the galaxy.
D) thickness of the disk.
E) presence of an active nucleus.
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