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Physical Review Letters|October 11, 2011
Revealing the physics of R modes in low-mass x-ray binariesWynn C G Ho, Nils Andersson, Brynmor HaskellScience Advances|November 25, 2015
Pinning down the superfluid and measuring masses using pulsar glitchesWynn C G Ho, Cristóbal M Espinoza, Danai Antonopoulou, et al.Monthly Notices of the Royal Astronomical Society|November 5, 2020
Return of the Big Glitcher: NICER timing and glitches of PSR J0537-6910Wynn C G Ho, Cristóbal M Espinoza, Zaven Arzoumanian, et al.Reports on Progress in Physics. Physical Society (Great Britain)|October 24, 2022
Pulsar glitches: observations and physical interpretationDanai Antonopoulou, Brynmor Haskell, Cristóbal M EspinozaPhilosophical Transactions. Series A, Mathematical, Physical, and Engineering Sciences|April 18, 2018
Gravitational waves from neutron stars and asteroseismologyWynn C G HoPhysical Review Letters|August 26, 2003
Polarized x-ray emission from magnetized neutron stars: signature of strong-field vacuum polarizationDong Lai, Wynn C G HoNature|November 6, 2009
A neutron star with a carbon atmosphere in the Cassiopeia A supernova remnantWynn C G Ho, Craig O HeinkePhysical Review Letters|April 28, 2009
Hydrodynamical trigger mechanism for pulsar glitchesKostas Glampedakis, Nils AnderssonLiving Reviews in Relativity|February 10, 2017
Relativistic Fluid Dynamics: Physics for Many Different ScalesNils Andersson, Gregory L ComerEntropy (Basel, Switzerland)|August 29, 2024
A Field-Theory Approach for Modeling Dissipative Relativistic FluidsNils Andersson, Thomas Celora, Gregory Comer, et al.Pageof 2