18 citations · 27 across the 2 of their papers we have counts for
5 papers · 1 filter
Acceleration and Transport of the Unstable Cosmic-ray Isotope Fe in Supernova-Enriched Environments
Xin-Yue Shi, Martin Pohl, Michael M. Schulreich
The unstable isotope Fe, with a half-life of 2.6 million years, is produced primarily in supernova explosions. The observed presence of Fe in cosmic rays and its dete…
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…
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 plerionic rectangular supernova remnants of static progenitors
Meyer D. M. -A., Meliani Z., Velazquez P. F. +2
Pulsar wind nebulae are a possible final stage of the circumstellar evolution of massive stars, where a fast rotating, magnetised neutron star produces a powerful wind that interac…
Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment
O. Petruk, T. Kuzyo, S. Orlando +5
We present very-high-resolution 1D MHD simulations of the late-stage supernova remnants (SNR). In the post-adiabatic stage the magnetic field has an important and significant dynam…