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Objects which have contracted, but are of too little mass to establish thermonuclear reactionsin their cores, are ________, which slowly continue to cool.

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Most stars in our part of the Galaxy are formed:


A) alone.
B) in open clusters of a few dozen.
C) in associations of thousands of stars across a spiral arm of the Galaxy.
D) in globular clusters of millions of stars.
E) in a singular event just after the Big Bang.

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To deduce the interior conditions of the dense regions in which stars form, it is necessary forastronomers to observe in the ________ part of the spectrum.

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Type M stars evolve to the main sequence faster than our G type Sun.

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Most stars in the Milky Way probably formed:


A) alone.
B) in intergalactic space, then were swept up into the Galaxy.
C) in clusters in the Galaxy's spiral arms.
D) from planetary nebulae.
E) in the galactic Nucleus, then migrated outward later.

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How long does it take an O-type star to form, compared to the time for a solar-type star toform?


A) 1/300 as long
B) 1/30 as long
C) about the same time
D) 30 times longer
E) 300 times longer

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During the Kelvin-Helmholtz contraction phase, a protostar has a much ________ brightnessas compared to the Sun.

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Our Sun, along with most of the stars in our neighborhood, probably formed:


A) a few million years ago.
B) about 10 million years ago.
C) hundreds of millions of years ago.
D) billions of years ago.
E) at the beginning of the universe.

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A newly formed protostar will radiate primarily at which wavelength?


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

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What is the force that keeps a main sequence star from blowing apart?


A) magnetism
B) gravitation
C) the strong force
D) radiation pressure
E) electron degeneration pressure

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Stage 4 of star formation is when the object can exhibit violent surface activity producingextremely strong protostellar winds. This phase is also called the:


A) protostar phase.
B) Herbig-Haro phase.
C) brown dwarf phase.
D) T Tauri phase.
E) protoplanetary nebula phase.

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Collisions between galaxies tend to destroy, not create, stars.

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Rotation causes the cocoon of dust to flatten into a dusty disk around protostars.

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More massive stars are able to form in a(n)________ time than less massive stars.

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Why does the term "planet" have a different meaning when applied to brown dwarfs than inour solar system?

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In our solar system, a planet is a large...

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After stage 3 in star formation, the protostar develops a surface better known as a(n)________.

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What do we mean by the term "molecular clouds"? Why do they exist? How can observationof their properties yield clues to the processes of stellar formation?

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Molecular clouds are very cool interstel...

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A cloud fragment too small to collapse into a main sequence star becomes a:


A) white dwarf.
B) pulsar.
C) T Tauri object.
D) brown dwarf.
E) planet of another star.

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During a protostar's T Tauri phase, it:


A) begins a period of reduced activity.
B) expands dramatically.
C) lies on the main sequence.
D) may develop very strong winds.
E) changes its spin direction.

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A protostar develops a bipolar flow of gas when it is still surrounded by an equatorial disk of________.

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