Wynn C. G. Ho

TL;DR: In this paper, a search for quasi-monochromatic gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537−6910 using data from the second and third observing runs of LIGO and Virgo was presented.

TL;DR: In this article, the authors present a detailed study of the young radio pulsar J1119-6127, which has a characteristic age of 1900yr and a spin-down-inferred magnetic field of 4.1e13G, and its associated supernova remnant G292.5, using deep XMM-Newton and Chandra X-ray Observatory exposures of over 120k from each telescope.

TL;DR: In this paper, the equation of state, polarization and radiation properties for nonideal, strongly magnetized plasmas which compose outer envelopes of magnetic neutron stars were studied and detailed calculations were performed for partially ionized hydrogen atmospheres and for condensed hydrogen or iron surfaces of these stars.

TL;DR: In this article, the authors used the magnetic field B and initial spin period P_0 inferred from supernova and gamma-ray bursts observations to obtain simple constraints on the dimensionless amplitude of the mountain of epsilon 10^-4 (B/10^14 G) (P_0/1 ms) or alpha > 0.01 (b/10+14 G), and found that the light curves are strongly affected, with a significant decrease in peak luminosity and increase in time to peak brightness.

TL;DR: In this article, the local dynamics of a realistic neutron star core, including composition gradients, superfluidity and thermal effects, were studied and the main focus was on the gravity g-modes which are supported by composition stratification and thermal gradients.