Marco Vetter
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View article: Magnetically driven outflows in the 3D common envelope evolution of massive stars
Magnetically driven outflows in the 3D common envelope evolution of massive stars Open
Recent three-dimensional magnetohydrodynamical simulations of the common envelope interaction have revealed the self-consistent formation of bipolar magnetically driven outflows. These outflows are launched from a toroidal structure that h…
View article: From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral
From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral Open
Self-consistent three-dimensional modeling of the entire common-envelope phase of gravitational wave progenitor systems until full envelope ejection is challenged by the vast range of spatial and temporal scales involved in the problem. Pr…
View article: Large-scale ordered magnetic fields generated in mergers of helium white dwarfs
Large-scale ordered magnetic fields generated in mergers of helium white dwarfs Open
Stellar mergers are one important path to highly magnetised stars. Mergers of two low-mass white dwarfs may create up to every third hot subdwarf star. The merging process is usually assumed to dramatically amplify magnetic fields. However…
View article: Large-scale ordered magnetic fields generated in mergers of helium white dwarfs
Large-scale ordered magnetic fields generated in mergers of helium white dwarfs Open
Stellar mergers are one important path to highly magnetised stars. Mergers of two low-mass white dwarfs may create up to every third hot subdwarf star. The merging process is usually assumed to dramatically amplify magnetic fields. However…
View article: Evolution and final fate of massive post-common-envelope binaries
Evolution and final fate of massive post-common-envelope binaries Open
Mergers of neutron stars (NSs) and black holes (BHs) are nowadays observed routinely thanks to gravitational-wave (GW) astronomy. In the isolated binary-evolution channel, a common-envelope (CE) phase of a red supergiant (RSG) and a compac…
View article: Evolution and final fate of massive post-common-envelope binaries
Evolution and final fate of massive post-common-envelope binaries Open
Mergers of neutron stars (NSs) and black holes (BHs) are nowadays observed routinely thanks to gravitational-wave (GW) astronomy. In the isolated binary-evolution channel, a common-envelope (CE) phase of a red supergiant (RSG) and a compac…