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A star on the main sequence has 7 solar masses. The star will evolve into a _____ _______ and its core will be supported by ___ _____ ______.


A) white dwarf, electron degeneracy pressure
B) neutron star, neutron degeneracy pressure
C) black hole, no pressure (i.e., it will not be supported)
D) white dwarf, neutron star, or black hole; electron degeneracy, neutron degeneracy, and no pressure, respectively.

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

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  Using the above graph of modulated light from a pulsar, how many planets can you determine to be in this system? A)  0 B)  1 C)  2 D)  3 Using the above graph of modulated light from a pulsar, how many planets can you determine to be in this system?


A) 0
B) 1
C) 2
D) 3

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

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For a point mass equal to that of the Sun, how far does the Schwarzschild radius extend from its center?


A) A few kilometers away
B) A few solar radii away
C) A few astronomical units (AU) away
D) A few parsecs away

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

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To tell the difference between a neutron star and a black hole in an X-ray binary, we must find the temperature of the object.

A) True
B) False

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How are neutron stars and white dwarfs similar?

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They are both compact objects,...

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Why might we suspect that a black hole in a binary system could emit X-rays?

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If matter flows into a black h...

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Which of the following objects is considered to possibly contain a black hole?


A) the central star of the Crab nebula
B) the Orion nebula.
C) LMC X-3
D) Algol
E) PSR 1257+12

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

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An isolated black hole in space would be difficult to detect because


A) there would be no light source nearby.
B) it would not be rotating rapidly.
C) it would be stationary.
D) very little matter would be falling into it.
E) there would be very few stars behind it whose light the black hole could block out.

F) A) and D)
G) All of the above

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What observational evidence do we have that black holes exist?

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An isolated black hole in space will not...

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The stability of a neutron star is expected only if a neutron star is a ____________.


A) solid
B) fluid
C) gas
D) All of the other choices are correct.

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

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If the inner accretion disk around a black hole has a temperature of 106 K, at what wavelength will it radiate the most energy? ( Hint : From Wien's law, λ T =3,000,000 where λ is in nm and T is in K.)


A) 106 nm
B) 3 nm
C) 3 × 106 nm
D) 1 nm
E) 3 × 1011 nm

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

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   In the lighthouse model shown above, the light bulb represents the neutron star. In the lighthouse model shown above, the light bulb represents the neutron star.

A) True
B) False

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None of the pulsars emit pulses of visible light because


A) pulsars are too hot to emit visible light.
B) pulsars contain black holes that won't let visible light escape.
C) the gravitational field of a pulsar is so great that the visible light emitted is redshifted.
D) pulsars are too far away for the visible light to be bright enough to be detected at Earth.
E) A few pulsars do emit visible light pulses.

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

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What happens when a core's mass exceeds 3 solar masses and its density exceeds that which electron degeneracy pressure can support?


A) The core collapses into a black hole.
B) The core collapses into a neutron star.
C) The core collapses into a white dwarf.
D) The core collapses into a neutron star or a black hole.

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

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The material that accretes onto a neutron star or black hole is expected to emit X-rays because


A) the material will produce synchrotron radiation.
B) hydrogen nuclei begin to fuse and emit high-energy photons.
C) the material will become hot enough that it will radiate most strongly at X-ray wavelengths.
D) as the material slows down it converts thermal energy to gravitational potential energy.
E) None of the other choices are correct.

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

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Although neutron stars are very hot, they are faint and not easy to see at visual wavelengths because


A) light does not escape from their event horizon.
B) most lie beyond dense dust clouds.
C) they have only a small surface area from which to emit.
D) the peak of their thermal emission is at much shorter wavelengths than visual.
E) they have only a small surface area from which to emit and the peak of their thermal emission is at much shorter wavelengths than visual.

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

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Pulsars cannot be spinning white dwarfs because


A) white dwarfs are not that common.
B) white dwarfs are not dense enough.
C) white dwarfs do not have magnetic fields.
D) a white dwarf spinning that fast would fly apart.
E) All of the other choices are correct.

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

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Unseen objects in our galaxy have been found by the bending effect they have on more distant stars' light passing near them. These small objects that don't emit light are calculated to have masses of about 10 × the mass of the Sun. Which is the best choice for these objects?


A) black hole
B) neutron star
C) white dwarf
D) main-sequence stars

E) All of the above
F) None of the above

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Why does our theory predict that neutron stars will spin rapidly?

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The principle of conservation of angular...

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___ _____ _ occurs when light travels out of a gravitational field, loses energy, and its wavelength grows longer.


A) A gravitational blue shift
B) The solar wind
C) A gravitational redshift
D) A X-ray burst
E) A pulsar wind

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

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