33 citations · 146 across the 9 of their papers we have counts for
4 papers · 1 filter
Mixing of materials in magnetised core-collapse supernova remnants
Meyer D. M. -A., Pohl M., Petrov M. +1
Core-collapse supernova remnants are structures of the interstellar medium (ISM) left behind the explosive death of most massive stars (smaller or equal to 40 Mo). Since they resul…
3D MHD astrospheres: applications to IRC-10414 and Betelgeuse
D. M. -A. Meyer, A. Mignone, M. Petrov +3
A significative fraction of all massive stars in the Milky Way move supersonically through their local interstellar medium (ISM), producing bow shock nebulae by wind-ISM interactio…
On the ring nebulae around runaway Wolf-Rayet stars
D. M. -A. Meyer, L. M. Oskinova, M. Pohl +1
Wolf-Rayet stars are advanced evolutionary stages of massive stars. Despite their large mass-loss rates and high wind velocities, none of them display a bow shock, although a fract…
Wind nebulae and supernova remnants of very massive stars
D. M. -A. Meyer, M. Petrov, M. Pohl
A very small fraction of (runaway) massive stars have masses exceeding - and are predicted to evolve as Luminous-Blue-Variable and Wolf-Rayet stars before e…