Her X-1 precession implies unpinned crustal superfluid vortices with weak mutual friction persisting for centuries.
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A modified ellipsoidal modulation model with precessing disk irradiation effects revises the SMC X-1 pulsar mass to approximately 1.35 solar masses.
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Theoretical Constraints on Neutron Star Superfluidity from Her X-1 Precession
Her X-1 precession implies unpinned crustal superfluid vortices with weak mutual friction persisting for centuries.
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Optical Super-orbital Modulation of SMC X-1: Disk Precession and a Revised Pulsar Mass
A modified ellipsoidal modulation model with precessing disk irradiation effects revises the SMC X-1 pulsar mass to approximately 1.35 solar masses.