Neutron stars host the strongest magnetic fields that we know of in the Universe. Their
magnetic fields are the main means of generating their radiation, either magnetospheric or …

By combining relativistic mean field models and equivparticle models with density-
dependent quark masses, we construct explicitly “a quark Fermi sea” and “a baryonic Fermi …

In the framework of the Thomas-Fermi approximation, we systematically study the EOSs and
microscopic structures of neutron star matter in a vast density range with nb≈ 10− 10-2 fm …

We derive the initial spin period distribution of neutron stars by studying the population of
young pulsars associated with supernova remnants. Our hierarchical Bayesian approach …

Pulsars have long been studied in the electromagnetic spectrum. Their environments are
rich in high-energy cosmic-ray electrons and positrons likely enriching the interstellar …

High precision mapping of HO megamaser emission from active galaxies has revealed more
than a dozen Keplerian HO maser discs, which enable a 4 per cent uncertainty estimate of …

We report the independent discovery of PSR J0026-1955 with the Murchison Widefield
Array (MWA) in the ongoing Southern-sky MWA Rapid Two-metre pulsar survey. J0026 …

Considering the effects of charge screening, we propose a new numerical recipe within the
framework of the Thomas-Fermi approximation, where the properties of nuclear matter …

We explore the effects of strangeness and Δ resonance in baryonic matter and compact
stars within the relativistic-mean-field models. The parameter set PKDD is adopted for NN …

We report new Chandra X-ray observations of the shell supernova remnant Kes 75 (G29. 7−
0.3) containing a pulsar and pulsar-wind nebula (PWN). Expansion of the PWN is apparent …