Neutron stars are sometimes found in binary systems, where matter overflowing from a companion star and accreting onto the neutron star will produce X-rays and other energetic phenomena.
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Q3: An 8M
Q4: Pulsating variable stars are more commonly known
Q5: The production of large numbers of neutrons
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Q7: We can determine the age of a
Q9: The CNO cycle is the dominant mechanism
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