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A galaxy rotation curve is a plot of the rotation speed as a function of the:


A) galaxy's luminosity
B) mass of the dark matter halo
C) brightness of the luminous matter in the galaxy
D) radius from the center
E) ages of star clusters

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Elliptical galaxies contain hot gas that is heated by supernova explosions.

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What determines the three-dimensional shapes of galaxies?

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The velocities of st...

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The unified model of AGN suggests that quasars,Seyfert galaxies,and radio galaxies:


A) are unrelated,although they are all very luminous galaxies at radio wavelengths
B) are powered by similar mass accretion rates onto supermassive black holes
C) are driven by violent mergers of two gas-rich spiral galaxies
D) are similar phenomena but viewed from different orientation angles
E) are all powered by high rates of star formation and supernova explosions

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Stars in the disks of spiral galaxies have orbits that:


A) are randomly oriented
B) constantly are getting larger
C) mostly aligned in the same plane
D) spiral shaped
E) unaffected by dark matter

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How do we know that many E galaxies contain significant amounts of dark matter?

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Many E galaxies are observed to contain ...

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More luminous giant galaxies tend to have __________ supermassive black holes at their centers.


A) more massive
B) radio quiet
C) more luminous
D) slower rotating
E) less massive

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If the rotational speed of the gas in the disk of a spiral galaxy is 200 km/s at a distance of 25,000 pc from its center,then what is the mass enclosed within this radius?


A) 7.5 billion M
B) 18 billion M
C) 70 billion M
D) 230 billion M
E) 400 billion M

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If an AGN varies its brightness on a timescale of 4 hours,then what is the size of the AGN measured in AU?

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The size of the AGN is the distance that...

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If elliptical galaxies do not have cold gas clouds for which we can measure the Doppler shift,then how can we measure the mass of an elliptical galaxy?


A) by measuring the speeds of stars in the nucleus
B) by observing the velocity of the hot,X-ray emitting gas that surrounds the galaxy
C) by measuring the number of H II regions in the galaxy
D) by measuring how many supernovae go off each century
E) by measuring the amount of blue light in the galaxy

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The type of AGN we see depends mostly on the angle at which we view the galaxy.

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If a galaxy had no dark matter,how would the velocity (v) of a star that orbited far outside the visible extent of the galaxy depend on its distance (r) from the center of the galaxy?


A) ν ∝ r2
B) ν ∝ r1
C) ν ∝ If a galaxy had no dark matter,how would the velocity (v) of a star that orbited far outside the visible extent of the galaxy depend on its distance (r) from the center of the galaxy? A) ν ∝ r<sup>−</sup><sup>2</sup> B) ν ∝ r<sup>−</sup><sup>1</sup> C) ν ∝   D) ν ∝ r E) ν ∝ r<sup>2</sup>
D) ν ∝ r
E) ν ∝ r2

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The disks of spiral galaxies appear blue because:


A) they are moving toward us
B) they contain a relatively high concentration of low-mass stars
C) they contain active regions of star formation
D) they contain more metals that,when ionized,emit blue light
E) stars collide with each other frequently in these dense regions and explode as Type I supernovae

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Approximately __________ of spiral galaxies are barred.


A) 10 percent
B) 25 percent
C) 35 percent
D) 50 percent
E) 75 percent

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The Hubble diagram is a way of sorting galaxies by their visual appearance.

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Give three examples of types of active galactic nuclei and give one reason why each is unique.

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Three types of AGNs: (1)quasars-extremel...

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What is plotted on a rotation curve,and what can it tell us about a galaxy?

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A rotation curve is a plot of the veloci...

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The image below was probably taken in ____________ wavelengths because _______________________. The image below was probably taken in ____________ wavelengths because _______________________.   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


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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We interpret the fact that we saw more AGNs in the past than we do today to indicate that:


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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What happens to active galaxies when their AGNs run out of fuel?


A) The black holes powering them collapse even further.
B) They simply become normal galaxies.
C) They slowly dissipate into clouds of gas and dust.
D) They eventually pull in material from farther out,starting the AGN process all over again.
E) They explode as gamma-ray bursts.

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