CDF-S XT1 and XT2 are both interpreted as X-ray counterparts of binary neutron star mergers with newborn magnetars, seen from the trapped and free zones respectively.
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A unified binary neutron star merger magnetar model for the Chandra X-ray transients CDF-S XT1 and XT2
CDF-S XT1 and XT2 are both interpreted as X-ray counterparts of binary neutron star mergers with newborn magnetars, seen from the trapped and free zones respectively.