Wynn C. G. Ho

TL;DR: In this article, a model of a buried magnetic field was proposed to explain the youth and low observed magnetic field of the central compact objects, which is a newly emerging class of young neutron stars near the center of supernova remnants.

TL;DR: In this article, the authors analyzed NICER and XMM-Newton observations of RX J1605.3+3249, in order to address its timing and spectral behavior, finding no significant pulsation with pulsed fraction higher than 1.3% (3σ) for periods above 150 ms.

TL;DR: In this paper, the authors study the impact of the mass and radius of a 1.4 solar mass neutron star on the EOS of a binary binary neutron star, and show that the new NICER results provide tight constraints for the pressure of neutron star matter at around twice saturation density, which shows the power of these observations to constrain dense matter interactions at intermediate densities.

TL;DR: In this paper, the authors re-analysed Chandra X-ray observations of the bright supernova remnant (SNR) 1E 0102.2-7219 in the Small Magellanic Cloud, to validate the detection of a neutron star (NS) in the SNR by Vogt et al.

TL;DR: The first rotation powered pulsars were discovered in the Small Magellanic Cloud (SMC) in more than a decade as discussed by the authors, using a Parkes Multi-Beam (PMB) survey of MCSNR J0127-7332.