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What compelling evidence links pulsars to neutron stars?


A) Both pulsars and neutron stars can be found in globular star clusters.
B) Pulsars are known to evolve into neutron stars.
C) Only a small, very dense source could rotate that rapidly without flying apart.
D) Pulsars are always found in binary systems with neutron stars.
E) Both pulsars and neutron stars have been discovered near the Sun.

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In a nova, there is a white dwarf, an evolving companion star, and a(n) ________ surrounding the white dwarf's equator.

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Except for hydrogen and most of the helium, all the elements have been formed through stellar nucleosynthesis.

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Whose work with SETI lead to the discovery of pulsars in 1967?


A) Jocelyn Bell
B) Sir Bernard Lovell
C) Anthony Hewish
D) Martin Schwarzschild
E) Stephen Hawking

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What are two differences observed between Type I and Type II supernovae?

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Type I supernovae have very little hydro...

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What is the reason a type-I supernova slows its dimming after about 2 months?


A) The planetary nebula cooled enough to form a dust shell.
B) Energy is released from the decay of radioactive cobalt 56 to iron 56.
C) The supernova remnant suddenly becomes transparent.
D) The burst of energy carried by neutrinos is finally observed.
E) Energy from the supernova's shock wave is released as it hits interstellar matter.

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What would happen if mass is added to a 1.4 solar mass white dwarf?


A) The star would explode as a nova.
B) The star's radius would increase.
C) The star would immediately collapse into a black hole.
D) The star would erupt as a carbon detonation (type I) supernova.
E) The core would collapse as a type II supernova.

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What role does the main sequence mass of the star play in the formation of heavy elements in the giant stage?

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Basically the greater the mass of the at...

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What direct evidence do astronomers have that supports the heavy element formation in stars?


A) The presence of technetium in giant star spectra
B) Observed elemental abundances
C) Gamma-ray emissions from decay of cobalt 56 in supernovae
D) Light curves of type-I supernovae
E) All of the above are evidence of this.

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Why is the post-Main Sequence structure of a high mass star sometimes described by an "onion-layer" model? Explain.

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Late in the evolution of massive stars, ...

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The central star of the Crab Nebula has now collapsed into a ________, whose energy keeps this famous nebula visible even in binoculars.

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Type I supernovae result from ________ stars which have accreted sufficient additional mass via mass transfer from a close binary companion.

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Supernova remnants differ from star forming regions because, although there is ionized hydrogen in both, supernova remnants


A) don't look like star forming regions.
B) are much bigger than star forming regions.
C) are located far from star forming regions.
D) are more diffuse than star forming regions.
E) contain no ionizing stars.

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Newly formed neutron stars have weak magnetic fields which strengthen over time, due to the conservation of angular momentum.

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Like most pulsars, the Crab Nebula neutron star is known only by its radio pulses.

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Under what circumstances will a nova occur?

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When a white dwarf pulls mass off its co...

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Gamma-ray bursts seem to come primarily from neutron star binaries in the plane of our own Milky Way Galaxy.

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A hypernova creates


A) a black hole.
B) a pulsar.
C) a neutron star.
D) short-duration gamma-ray bursts.
E) Both B and C are correct.

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If successive generations of stars return material back to the interstellar medium which is enriched in heavier elements, then we expect that old stars are ________ compared to younger stars.

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A recurring nova could eventually explode as a Type I supernova.

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