3 papers
astro-ph.HE2026
Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
A. De Sarkar, D. F. Torres, B. Olmi +2
Pulsar wind nebulae (PWNe) constitute the largest population of Galactic very-high-energy (VHE; GeV) -ray sources and are key laboratories for studying particle accel…
astro-ph.HE2026
Population synthesis of Galactic middle-aged pulsar wind nebulae II. Observational signatures of superefficiency
D. F. Torres, A. De Sarkar, B. Olmi +2
Pulsar wind nebulae (PWNe) interacting with the host supernova remnants (SNRs) can enter the reverberation phase in which reverse-shock-driven compression amplifies the magnetic fi…
astro-ph.HE2026
Classical, large scale 3D MHD simulations of interacting pulsar wind nebulae
D. M. -A. Meyer, D. F. Torres
Magnetized rotating neutron stars, or pulsars, are a possible end product of massive star evolution. Their relativistic wind successively interacts with the supernova ejecta of the…