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True/False
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Multiple Choice
A) supernova of Type II
B) nova
C) planetary nebula
D) brown dwarf
E) supernova of Type I
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True/False
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Multiple Choice
A) no, or we would see them as the majority of naked- eye stars
B) no, it will lose so much mass as to cross the Chandrasekhar Limit
C) yes, before and after the helium flash
D) yes, before and after the Type II supernova event
E) no, the planetary nebula blows off all the outer shells completely
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True/False
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True/False
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True/False
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Multiple Choice
A) a Type II supernova
B) a nova
C) a Type I supernova
D) All of these need mass transfer to occur.
E) None of these depends on mass transfer.
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Multiple Choice
A) It did not produce the flood of neutrinos our models had led us to expect.
B) The parent star was a blue supergiant, much like Deneb or Rigel.
C) The supernova was luminous enough to see with the naked eye.
D) Its pulsar appeared within weeks of the explosion.
E) The supernova was not even in our own Galaxy.
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A) very common, making up the majority of the dark matter in the universe.
B) often made from very low mass protostars that never fuse hydrogen.
C) rare, for few binary systems are close enough for this merger to happen.
D) rare, for collapsing cores of over three solar masses are uncommon.
E) not found yet; the oldest, coldest white dwarf in the Galaxy has not cooled enough yet.
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Multiple Choice
A) the total number of main- sequence stars
B) the amount of dust that lies around the cluster
C) the ratio of giants to supergiants
D) the luminosity of the main- sequence turn- off point
E) the number of white dwarfs
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