Neutron star cooling in seven of eight transient outbursts from LMXBs is matched by thermonuclear heating leakage via an updated nscool boundary condition without ad hoc shallow heating.
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On a re-examination of neutron star cooling in transient sources -- No shallow heating required?
Neutron star cooling in seven of eight transient outbursts from LMXBs is matched by thermonuclear heating leakage via an updated nscool boundary condition without ad hoc shallow heating.