9 citations · 11 across the 9 of their papers we have counts for
10 papers
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…
Material mixing in pulsar wind nebulae of massive runaway stars
D. M. -A. Meyer, D. F. Torres
In this study we quantitatively examine the manner pulsar wind, supernova ejecta and defunct stellar wind materials distribute and melt together into plerions. We performed 2.5D MH…
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…
The backreaction of stellar wobbling on accretion discs of massive protostars
D. M. -A. Meyer, E. Vorobyov
In recent years, it has been demonstrated that massive stars see their infant circumstellar medium shaped into a large, irradiated, gravitationally unstable accretion disc during t…
Supernova remnants of red supergiants: from barrels to Cygnus loops
D M A Meyer, P F Velazquez, M Pohl +5
Core-collapse supernova remnants are the nebular leftover of defunct massive stars which have died during a supernova explosion, mostly while undergoing the red supergiant phase of…
On the origin of mixed morphology supernova remnants: Linking their properties to the evolution of a red supergiant progenitor star
Alexandros Chiotellis, Emmanouil Zapartas, Dominique M. -A. Meyer
Mixed-morphology supernova remnants (MMSNRs) are characterized by a shell-like morphology in the radio and centrally-peaked thermal emission in the X-ray band. The nature of this p…
Simulated non-thermal emission from SNR G1.9+0.3
Marco A. Villagran, D. O. Gómez, P. F. Velázquez +7
Supernova remnants are the nebular leftover of defunct stellar environments, resulting from the interaction between a supernova blastwave and the circumstellar medium shaped by the…