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Explain what keeps the nuclear reactions in a star under control; i.e., what would happen if too large an amount of energy is released in the center

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If the star makes slightly too much ener...

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  -The above image is an example of a/an ____________.  A) cluster of stars producing reflection nebula B) T association C) OB association D) Trapezium cluster -The above image is an example of a/an ____________.


A) cluster of stars producing reflection nebula
B) T association
C) OB association
D) Trapezium cluster

E) B) and C)
F) A) and D)

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What observations demonstrate the existence of an interstellar medium

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One way to investigate properties of the...

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_________ are small luminous nebulae excited by nearby young stars.


A) T Tauri stars
B) Herbig-Haro objects
C) O associations
D) Bok Globule
E) Giant molecular clouds

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

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What causes the outward gas pressure that balances the inward pull of gravity in a main-sequence star


A) the rapid outward flow of gas
B) the rapid inward flow of the gas
C) the high temperature of the gas
D) the high density of the gas
E) the high temperature and the high density of the gas

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

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Some young star clusters contain large numbers of protostars.

A) True
B) False

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In the collapse of a protostar ____________________ energy is converted to ____________________ energy.

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Why are massive stars more luminous than low mass stars That is, why is there a mass-luminosity relation

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To understand the mass-luminosity relati...

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How long can a 1-solar-mass star live


A) 0.5 solar lifetimes
B) 1 solar lifetime
C) 2 solar lifetimes
D) 10 solar lifetimes

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

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A(n) ____________________ is a cool, dense cloud of dust and gas that is undergoing gravitational contraction.

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The lowest-mass object that can initiate thermonuclear fusion of hydrogen has a mass of about


A) 1 solar masses.
B) 80 solar masses.
C) 8 solar masses.
D) 0.08 solar masses.
E) 0.001 solar masses.

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

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The creation of ________ require(s) that a young hot star (T ≈ 25,000 K) be relatively nearby.


A) emission nebulae
B) HI regions
C) molecular clouds
D) the cool gas of the interstellar medium
E) 21-cm radiation

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

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Absorption lines due to interstellar gas


A) are wider than the lines from stars because the gas is hotter than most stars.
B) are narrower than the lines from stars because the gas has a lower pressure than stars.
C) indicate that the interstellar medium contains dust.
D) indicate that the interstellar medium is expanding away from the Sun.
E) None of the other choices are correct.

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

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in the following cartoon image of Orion, where would you find the Orion nebula in the following cartoon image of Orion, where would you find the Orion nebula   A) below the belt (i.e., three white stars)  but above the lower right blue and lower left white stars B) above the belt (i.e., three white stars)  but below the upper red and the upper white stars C) in the belt, that is, among the three white stars D) outside the white lines


A) below the belt (i.e., three white stars) but above the lower right blue and lower left white stars
B) above the belt (i.e., three white stars) but below the upper red and the upper white stars
C) in the belt, that is, among the three white stars
D) outside the white lines

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

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The lower edge of the main-sequence band is known as ________ and represents the location in the H-R diagram at which stars begin their lives as main-sequence stars.


A) the Coulomb barrier
B) hydrostatic equilibrium
C) the birth line
D) the zero-age main sequence
E) the evolutionary track

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

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What evidence indicates protostars have formed


A) jets
B) bipolar outflows
C) protostellar disks
D) All of the other choices are correct.

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

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Due to the dust in the interstellar medium, a distant star will appear to an observer on Earth to be


A) brighter and cooler than it really is.
B) brighter and hotter than it really is.
C) fainter and cooler than it really is.
D) fainter and hotter than it really is.
E) unchanged in brightness or apparent color.

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

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Energy transport by ____________________ is important when photons cannot readily travel through a gas.

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A ZAMS star evolves __________ and to the __________ on the H-R diagram because ________________.


A) downward, left, the core expands which causes the outer layers to expand
B) upward, right, the core contracts which causes the outer layers to expand
C) upward, left, the core expands which causes the outer layers to contract
D) downward, right, the core contracts which causes the outer layers to contract

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

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  -The above image is a/an _________ wavelength image of a reflection nebula.  A) infrared B) visual C) radio D) X-ray -The above image is a/an _________ wavelength image of a reflection nebula.


A) infrared
B) visual
C) radio
D) X-ray

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

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