A) Galaxy A. It has to contain more luminous objects if we can see them individually, and so the galaxy as a whole has to be more luminous.
B) Galaxy A. The lumpiness means that there is a lot of dust in the galaxy, which absorbs some of the starlight. Therefore the total amount actually emitted must be larger, if it is to have the same brightness as the other galaxy.
C) Neither. If they have the same apparent size and brightness, they must be at equal distances.
D) Galaxy B. This galaxy appears smooth because it is farther away and the light from its stars all blends together. Because it is farther away, it has to be more luminous.
E) Galaxy B. The smooth light distribution means that the stars are moving around very quickly. Therefore the galaxy has more mass and is more luminous.
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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 primarily hidden by large amounts of cold gas and dust
E) AGNs had bigger central black holes in the past
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True/False
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Multiple Choice
A) Quasars and Seyfert galaxies are stellar-like sources.
B) Their brightness varies by factors of a few.
C) The emission lines in their spectra show gas rotating at speeds of thousands of km/s.
D) Their brightness varies on timescales ranging from hours to a day.
E) We can measure their angular size, which gives us the physical size when we know the distance.
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Multiple Choice
A) They are very far away.
B) They are moving away from us.
C) They have rapid internal motions.
D) They are very dense.
E) They have few heavy elements.
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Essay
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View Answer
Multiple Choice
A) rotates at the same speed as the gas in the disk
B) rotates at a speed that is different than the gas in the disk
C) stays constant in time as the gas in disk rotates through it
D) rotates backward compared to the stellar orbits
E) must only last a short time, since few galaxies with disks show spiral patterns
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True/False
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Multiple Choice
A) change constantly
B) are very large in size
C) are equal in all directions
D) are constant in time
E) are orientated in random in directions
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True/False
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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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Multiple Choice
A) radio; the disk probably contains many planets with intelligent life, who are beaming out radio and television signals into space
B) infrared; the central regions are bright, and cool stars in the bulges emit a lot of infrared light
C) visible; there is a lot dust in this galaxy that blocks light in a ring about halfway along the disk
D) ultraviolet; the light from hot young stars is mainly found along spiral arms
E) X-ray; the central nucleus is easily seen, and AGN emit a lot of X-rays
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Essay
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View Answer
Essay
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True/False
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Multiple Choice
A) 1 * 1011 M
B) 2 * 1011 M
C) 8 *1011 M
D) 1 * 1012 M
E) 4 * 1012 M
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Multiple Choice
A) 5 percent
B) 25 percent
C) 33 percent
D) 50 percent
E) 90 percent
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True/False
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Multiple Choice
A) We know that massive stars make black holes, and most galaxies contain a lot of massive stars.
B) We know black holes are made of dark matter, and galaxies are mostly made up of dark matter.
C) We know that black holes emit radio waves, and many AGNs are bright at radio waves.
D) We measure that the mass of the black hole is increasing as material falls into it.
E) In some systems, we can see both redshifted and blueshifted emission lines from material orbiting around the black hole.
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Multiple Choice
A) the spiral merges with another galaxy
B) the galaxy is young
C) the galaxy's disk is regularly disturbed
D) the galaxy absorbs a satellite galaxy
E) a supernova explosion takes place
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