Chandra non-detection of PSR J0901-4046 yields Lx limits comparable to neutron-star spin-down power but four orders of magnitude below white-dwarf spin-down power, disfavoring an isolated white-dwarf engine.
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Long-period radio transient PSR J0901-4046 is not an Isolated White Dwarf Pulsar
Chandra non-detection of PSR J0901-4046 yields Lx limits comparable to neutron-star spin-down power but four orders of magnitude below white-dwarf spin-down power, disfavoring an isolated white-dwarf engine.