In a neutron star, the protons and electrons are fused together, leaving only neutrons.
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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
Q20: A neutron star is what can remain
Q21: An object more massive than the Sun,
Q22: No optical traces have been found of
Q23: No communication is possible across an event
Q24: Some gamma- ray bursters may be due
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