The production of large numbers of neutrons in nuclear reactions at the core of a massive star helps rob the core of energy and speeds its eventual collapse.
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Q1: The principal means by which high-mass stars
Q2: The nuclear reaction that produces most of
Q3: An 8M
Q4: Pulsating variable stars are more commonly known
Q6: We can determine the age of a
Q7: We can determine the age of a
Q8: Neutron stars are sometimes found in binary
Q9: The CNO cycle is the dominant mechanism
Q10: Most of the uranium (atomic mass= 238)
Q11: A main-sequence star of 25 solar masses
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