9 citations · 11 across the 8 of their papers we have counts for
5 papers · 1 filter
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 accele…
Runaway stars and the Galactic supernova remnant landscape: non-thermal emission and observational evidence
Rowan Batzofin, Kathrin Egberts, Dominique M. -A. Meyer +1
Context. A significant fraction (~30%) of massive stars in our Galaxy are moving supersonically through the interstellar medium, which strongly governs their location at the time t…
3D MHD simulations of runaway pulsars in core collapse supernova remnants
D. M. A. Meyer, D. F. Torres, Z. Meliani
Pulsars are one of the possible final stages in the evolution of massive stars. If a supernova explosion is anisotropic, it can give the pulsar a powerful kick, propelling it to su…
Pulsar wind nebulae meeting the circumstellar medium of their progenitors
D. M. A. Meyer, Z Meliani, D. F. Torres
A significative fraction of high mass stars sail away through the interstellar medium of the galaxies. Once they evolved and died via a core collapse supernova, a magnetized, rotat…
Particle acceleration, escape and non-thermal emission from core-collapse supernovae inside non-identical wind-blown bubbles
Samata Das, Robert Brose, Martin Pohl +2
In the core-collapse scenario, the supernova remnants evolve inside the complex wind-blown bubbles, structured by massive progenitors during their lifetime. Therefore, particle acc…