In a neutron star, the electrons in the core are all in contact with each other.
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Q8: An X- ray burster is similar to
Q9: The pulses from a pulsar are most
Q10: While most pulsars slow down over time,
Q11: All neutron stars seen from Earth are
Q12: Gamma- ray bursters seem scattered randomly over
Q14: Stars of less than 8 solar masses
Q15: Neutron stars are 100,000 times denser than
Q16: Millisecond pulsars are never members of close
Q17: Planet- sized bodies have been detected around
Q18: Newly- formed neutron stars start with weak
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