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How do the current star-formation rates of spiral and elliptical galaxies compare?

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Spirals contain lots of dust and cold ga...

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The spectra of most galaxies tell us that


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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How did astronomers determine that elliptical galaxies are composed mostly of dark matter?


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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Dark matter is most likely made up of


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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What type of galaxy is shown in the figure below? What type of galaxy is shown in the figure below?   A)  a giant elliptical B)  an ordinary spiral galaxy C)  an irregular galaxy D)  a barred spiral E)  a dwarf elliptical


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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For the more distant quasars, the emission lines that would normally occur in the visible domain would be shifted into


A) UV.
B) X-rays.
C) gamma rays.
D) infrared.
E) radio.

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Dust in galaxies does not count as dark matter because


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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We interpret the presence of more AGNs in the past than 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 hidden primarily by large amounts of cold gas and dust.
E) AGNs had bigger central black holes in the past.

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The Tully-Fisher method of determination of distances to galaxies is based on the correlation between


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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The nearest known quasar shows a redshift of z = 0.0516, which means it is at a distance of


A) 220 Mpc.
B) 450 Mpc.
C) 100 Mpc.
D) 15,400 Mpc.
E) 100 kpc.

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If a galaxy has a recessional velocity of 50,000 km/s, at what wavelength will you observe the H α\alpha emission line? (Note that the rest wavelength of the H α\alpha emission line is 656.3 nm.)


A) 695.7 nm
B) 719.4 nm
C) 742.3 nm
D) 765.7 nm
E) 1,750 nm

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If you found a galaxy with an H α\alpha emission line that had a wavelength of 756.3 nm, what would be the galaxy's redshift? (Note that the rest wavelength of the H α\alpha emission line is 656.3 nm.)


A) 0.05
B) 0.07
C) 0.10
D) 0.13
E) 0.15

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Microquasars are scaled-down versions of quasars, the former being powered by accretion onto stellar-sized black holes, the material being provided by a companion star.The underlying mechanism seems to be very similar in both microquasars and their supermassive AGNs.Typical microquasars have luminosities that are ten orders of magnitude lower than ordinary quasars.What is the typical level of accretion rate in the two cases?

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Microquasars have luminosities 1010...

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What were the positions taken by Heber Curtis and Harlow Shapley in their "Great Debate," and how were both of them partially correct?

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Curtis believed in a smaller galaxy (rou...

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You see a galaxy in which the H α\alpha line (rest wavelength = 656.3 nm) is observed at a wavelength of 756.3 nm.What would be the observed wavelength of a particular helium line that has a rest wavelength of 1,083 nm?


A) 1,083 nm
B) 1,183 nm
C) 1,248 nm
D) 1,440 nm
E) 3,142 nm

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Type Ia supernovae have a peak luminosity of 3.7 x1036 W.If you discover a Type Ia supernovae in a distant galaxy that has a measured brightness of 9.5 x10-17 W/m2, then how far away is this galaxy? Note that 1 Mpc = 3.1 x1022 m.


A) 0.3 Mpc
B) 40 Mpc
C) 1,200 Mpc
D) 1,800 Mpc
E) 3,500 Mpc

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Describe the known properties of dark matter, and contrast it with "normal" matter.

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Our main evidence for dark matter comes ...

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Quasars were first discovered in which region of the electromagnetic spectrum?


A) X-ray
B) gamma-ray
C) radio
D) infrared
E) visible

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If there is a 4 million MSUN black hole at the center of our galaxy, why is our own galaxy not an AGN?

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There is currently no significant infall...

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In spiral galaxies, the size of the central bulge is correlated with the


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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