Wynn Ho
0000-0002-6089-6836
108 papers found
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Pulsar Glitches: The Crust is not Enough
More than meets the eye: magnetars in disguise
Deep X-Ray Observations of the Young High-Magnetic-Field Radio Pulsar J1119–6127 and Supernova Remnant G292.2–0.5
Rotational evolution of young pulsars due to superfluid decoupling
Erratum: Magnetars: super(ficially) hot and super(fluid) cool
Magnetars are super hot and super cool
Central compact objects and their magnetic fields
Constraining the physics of the r-mode instability in neutron stars with X-ray and ultraviolet observations
Neutron star atmosphere composition: the quiescent, low-mass X-ray binary in the globular cluster M28
Magnetars: super(ficially) hot and super(fluid) cool
Signatures of Photon-Axion Conversion in the Thermal Spectra and Polarization of Neutron Stars
Superfluid effects on gauging core temperatures of neutron stars in low-mass X-ray binaries
Hottest Superfluid and Superconductor in the Universe: Lessons from the Cooling of the Cassiopeia A Neutron Star
Revealing the Physics ofrModes in Low-Mass X-Ray Binaries
New Optical/Ultraviolet Counterparts and the Spectral Energy Distributions of Nearby, Thermally Emitting, Isolated Neutron Stars
Evolution of a buried magnetic field in the central compact object neutron stars
Cosmic Recycling of Millisecond Pulsars
Cooling neutron star in the Cassiopeia A supernova remnant: evidence for superfluidity in the core
Cooling rates of neutron stars and the young neutron star in the Cassiopeia A supernova remnant
Direct Observation of the Cooling of the Cassiopeia a Neutron Star
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