Pulsar winds shocked in the ambient medium produce spectacular nebulae observable from
the radio through γ‐rays. The shape and the spectrum of a pulsar wind nebula (PWN) …

Pulsars are remarkable objects that emit across the entire electromagnetic spectrum,
providing a powerful probe of the interstellar medium. In this study, we investigate the …

We review multiwavelength properties of pulsar wind nebulae created by supersonically
moving pulsars and the effects of pulsar motion on the pulsar wind nebulae morphologies …

Pulsar wind nebulae (PWNe) are a prominent class of very high energy (E> 0.1 TeV)
Galactic sources. Their γ-ray spectra are interpreted as due to inverse Compton scattering of …

Among dozens of young pulsar wind nebulae (PWNe), some have been detected in TeV γ-
rays (TeV PWNe), while others have not (non-TeV PWNe). The TeV emission detectability is …

HESS J1809–193 is an extended TeV γ-ray source and the origin of its γ-ray emission
remains ambiguous. The pulsar wind nebula (PWN) of PSR J1J1809–193 lying inside the …

We present a statistical study of the nonthermal X-ray emission of 27 young rotation-
powered pulsars (RPPs) and 24 pulsar wind nebulae (PWNe) using the Chandra and XMM …

The number of binaries containing black holes (BH) or neutron stars (NS) depends critically
on the fraction of binaries that survive supernova (SN) explosions. We searched for surviving …

We present integrated pulse profiles at 5 GHz for 71 pulsars, including eight millisecond
pulsars (MSPs), obtained using the Shanghai Tian Ma Radio Telescope. Mean flux densities …

We report the discovery of 70.5 ms pulsations from the X-ray source AX J1838. 0–0655
using the Rossi X-Ray Timing Explorer (RXTE). PSR J1838–0655 is a rotation-powered …