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Molecular clouds, which have temperatures of around 10 K, are best observed at ________ wavelengths.


A) X-ray
B) ultraviolet
C) optical
D) infrared
E) radio

F) A) and E)
G) B) and C)

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Magnetic fields inside a molecular cloud act to


A) inhibit gravitational collapse.
B) fragment the cloud into numerous cores.
C) modulate the temperature of the molecules.
D) increase the formation of dust grains.
E) increase the formation of protostars.

F) A) and B)
G) None of the above

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Dust in the ISM appears dark in ________ wavelengths and bright in ________ wavelengths.


A) visible; ultraviolet
B) infrared; radio
C) infrared; visible
D) radio; ultraviolet
E) visible; infrared

F) All of the above
G) B) and C)

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Suppose we observe two molecular clouds containing dust.The dust in Cloud 1 peaks in emission at 50 mm, while the dust in Cloud 2 peaks in emission at 78 mm.How much warmer is the dust in Cloud 1 compared to Cloud 2?

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The peak of the emission is related to the dust temperature via Wien's law,so that T1 = 2,900 µm 11eadc6e_a8b3_cbbe_9b4c_e9adc521eafc_TB7448_11 and T2 = 2,900 µm 11eadc6e_a8b3_f2cf_9b4c_9156890b8051_TB7448_11 .The ratio of the two clouds' temperatures is then 11eadc6e_a8b3_f2d0_9b4c_65918057dd56_TB7448_11

What is the interstellar medium made of? Give rough percentages of each.

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The ISM is 99 percent gas and 1 percent ...

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Bipolar outflows create bright bow shocks because


A) the gas "piles up" when it encounters ultraviolet light.
B) the material collides with particles in the interstellar medium.
C) the star's magnetic fields trap the outflow material there.
D) the gas cools enough to allow H - ions to build up.
E) the outflows encounter newly forming planets.

F) A) and B)
G) A) and D)

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A protostar's evolutionary "track" in the H-R diagram traces


A) only how the protostar's radius changes with time.
B) how the protostar's luminosity, temperature, and radius change with time.
C) only how the protostar's luminosity changes with time.
D) only how the protostar's spectral type changes with time.
E) the protostar's location in the molecular cloud.

F) B) and C)
G) A) and D)

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Dust that glows with a peak emission wavelength of 40 μ\mu m has a temperature of


A) 10 K.
B) 72 K.
C) 100 K.
D) 120 K.
E) 1000 K.

F) A) and C)
G) A) and B)

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B

Compare the volume of the Sun with the volume of interstellar space it dominates.Is the occupied percentage large or small? Consider the volume around the Sun to be a sphere whose radius is equal to the distance to the nearest star, which is equal to 5 light-years.(Note: the radius of the Sun is 7 *105 km, and 1 light-year = 9.5 * 1012 km.)

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The volume occupied by the Sun is given ...

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Stars forming in molecular clouds tend to form first in


A) the low-density periphery.
B) the high-density core.
C) random locations.
D) any location where the temperature is highest.
E) the location with the heaviest elements.

F) A) and B)
G) A) and C)

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B

Star formation is an inefficient process, with only a few percent of the initial cloud fragment ending up as stars.This means the initial mass of a molecular cloud fragment that formed a 2 MSUN star was probably close to


A) 1 MSUN.
B) 50 MSUN.
C) 100 MSUN.
D) 5,000 MSUN.
E) 1,000,000 MSUN.

F) D) and E)
G) C) and D)

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How are Herbig-Haro objects related to T Tauri stars?

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Herbig-Haro objects are ionized gas form...

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Electronic transitions from the H2 molecule are easily seen at


A) X-ray wavelengths.
B) visible wavelengths.
C) radio wavelengths.
D) infrared wavelengths.
E) ultraviolet wavelengths.

F) A) and E)
G) A) and D)

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A young protostar is ________ than the Sun even though its surface temperature is ________.


A) less luminous; hotter.
B) larger; hotter.
C) smaller; the same.
D) more luminous; cooler.
E) smaller; hotter.

F) B) and D)
G) A) and B)

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What happens as a protostar contracts?


A) Its density rises.
B) Its temperature rises.
C) Its radius decreases.
D) Its pressure rises.
E) All of these are true.

F) A) and E)
G) C) and D)

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Dust that is heated to 30 K will emit a blackbody spectrum that peaks near


A) 1 µm.
B) 30 µm.
C) 50 µm.
D) 100 µm.
E) 500 µm.

F) B) and C)
G) A) and D)

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If you wanted to observe heavy elements in the interstellar medium, where would be the best place to look?


A) dust grains
B) cold gas
C) hot gas
D) warm gas
E) the interiors of forming protostars.

F) D) and E)
G) A) and B)

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The average density of the interstellar medium is


A) 1 atom/cm3.
B) 1,000 atoms/cm3.
C) 104 atoms/cm3.
D) 106 atoms/cm3.
E) 1012 atoms/cm3.

F) B) and C)
G) A) and D)

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Molecular cloud cores are places where you might find


A) protostars.
B) Herbig-Haro objects.
C) molecular hydrogen (H2) .
D) carbon monoxide (CO) .
E) all of these

F) B) and C)
G) None of the above

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How long does it typically take for a protostar to form a 1 MSUN star?


A) 3 *107 years
B) 3 * 105 years
C) 3,000 years
D) 300 years
E) 30 years

F) A) and C)
G) C) and E)

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