33 citations · 146 across the 9 of their papers we have counts for
10 papers
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…
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…
Rectangular core-collapse supernova remnants: application to Puppis A
D. M. -A. Meyer, P. F. Velazquez, O. Petruk +9
Core-collapse supernova remnants are the gaseous nebulae of galactic interstellar media (ISM) formed after the explosive death of massive stars. Their morphology and emission prope…
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…
Non-thermal radio supernova remnants of exiled Wolf-Rayet stars
D. M. -A. Meyer, M. Pohl, M. Petrov +1
A signification fraction of Galactic massive stars (> 8Mo) are ejected from their parent cluster and supersonically sail away through the interstellar medium (ISM). The winds of th…
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…
The early gaseous and stellar mass assembly of Milky Way-type galaxy halos
Gerhard Hensler, Mykola Petrov
How the Milky Way has accumulated its mass over the Hubble time, whether significant amounts of gas and stars were accreted from satellite galaxies, or whether the Milky Way has ex…
Can star cluster environment affect dust input from massive AGB stars?
Svitlana Zhukovska, Mykola Petrov, Thomas Henning
We examine the fraction of massive asymptotic giant branch (AGB) stars remaining bound in their parent star clusters and the effect of irradiation of these stars by intracluster ul…
Evolution of the Milky Way halo by accretion of dwarf satellite galaxies
Mykola Petrov, Gerhard Hensler
Within the Cold Dark Matter scenario the hierarchical merging paradigm is the natural result to form massive galactic halos by the minor mergers of sub-halos and, by this, inherent…