Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Although fifty years have passed since the discovery of radio pulsars, there is still no
satisfactory understanding of how these amazing objects operate. While there has been …

In this paper, we study compact binary millisecond pulsars with low-and very low-mass
companion stars (spiders) in the Galactic field, using data from the latest Gaia data release …

We present the final sample of 98 detached double white dwarf (WD) binaries found in the
Extremely Low Mass (ELM) Survey, a spectroscopic survey targeting< 0.3 M⊙ He-core WDs …

Abstract The Neutron star Interior Composition Explorer observed several rotation-powered
millisecond pulsars (MSPs) to search for or confirm the presence of X-ray pulsations. When …

We have produced a new software package for the simulation of pulsar populations,
PsrPopPy, based on the Psrpop package. The codebase has been re-written in Python …

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 …

At high-energy γ-rays (> 100 MeV), the Large Area Telescope (LAT) on the Fermi satellite
already detected more than 145 rotation-powered pulsars (RPPs), while the number of …

ABSTRACT A large sample of pulsars was observed as part of the Meterwavelength Single-
pulse Polarimetric Emission Survey. We carried out a detailed fluctuation spectral analysis …

In this review we describe recent observational and theoretical developments in our
understanding of pulsar winds and pulsar-wind nebulae (PWNe). We put special emphasis …