A) gas and dust
B) population I stars
C) stars associated with the spherical component of our galaxy
D) stars associated with the disk component of our galaxy
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Short Answer
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Multiple Choice
A) the existence of the nuclear bulge
B) the existence of the disk of the galaxy
C) the fact that the oldest stars in the galaxy are not metal-free
D) the difference in metal abundance of the population I and II stars
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Multiple Choice
A) They reveal that our galaxy is a grand design spiral.
B) They map the location of dense neutral hydrogen clouds.
C) They reveal that the Sun is currently located in the centre of a spiral arm.
D) They map the location of hot O and B stars by the radio radiation they emit.
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Not Answered
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Multiple Choice
A) +1
B) 0.0
C) -1.0
D) -3.5
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Not Answered
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True/False
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True/False
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Multiple Choice
A) They formed in the disk and were later ejected to the halo.
B) They built up over time from the collisions of stars in the halo.
C) They formed in other galaxies and were captured by close interactions.
D) They formed early on during the free-fall collapse of the proto-galactic material.
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True/False
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Multiple Choice
A) You will measure the wrong period.
B) You will think the Cepheid is farther away than it actually is.
C) You will think the Cepheid is closer than it actually is.
D) You will think the Cepheid is less luminous than it actually is.
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Multiple Choice
A) They are young and luminous.
B) They are old and have been part of the galaxy for a long time.
C) They are young and moving with large radial velocities.
D) They were formed in the galaxy's halo.
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Multiple Choice
A) All spiral arms would be gas- and dust-free.
B) All galaxies would have only two smooth spiral arms.
C) The Milky Way would show an irregular pattern of short arms.
D) The halo component of the Milky Way would show spiral arms as well.
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True/False
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Multiple Choice
A) Small velocities are seen at large distances from the galactic centre.
B) Small velocities are seen at distances close to the galactic centre.
C) Large velocities are seen at large distances from the galactic centre.
D) Large velocities are seen at distances close to the galactic centre.
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Essay
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