activity
20152025
most citedHow mergers magnetise massive stars

270 citations · 631 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR20251 cited

Magnetic field generation in mergers of massive main-sequence stars

Sebastian T. Ohlmann, Fabian R. N. Schneider, Friedrich K. Roepke +3

Magnetic fields are found in many astrophysical objects, ranging from galaxy clusters to the interstellar medium of galaxies and neutron stars. Strong surface magnetic fields are a…

astro-ph.SR20258 cited

Magnetically driven outflows in 3D common-envelope evolution of massive stars

Marco Vetter, Friedrich K. Roepke, Fabian R. N. Schneider +7

Recent three-dimensional magnetohydrodynamical simulations of the common-envelope interaction revealed the self-consistent formation of bipolar magnetically driven outflows launche…

astro-ph.SR2024

From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral

M. Vetter, F. K. Roepke, F. R. N. Schneider +4

Three-dimensional simulations usually fail to cover the entire dynamical common-envelope phase of gravitational wave progenitor systems due to the vast range of spatial and tempora…

astro-ph.SR2024

Large-scale ordered magnetic fields generated in mergers of helium white dwarfs

Rüdiger Pakmor, Ingrid Pelisoli, Stephen Justham +9

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 usual…

astro-ph.SR2020

Common-envelope evolution with an asymptotic giant branch star

C. Sand, S. T. Ohlmann, F. R. N. Schneider +2

Common-envelope phases are decisive for the evolution of many binary systems. Of particular interest are cases with asymptotic giant branch (AGB) primary stars, because they are th…

astro-ph.SR2020

Formation of sdB-stars via common envelope ejection by substellar companions

M. Kramer, F. R. N. Schneider, S. T. Ohlmann +4

Common envelope (CE) phases in binary systems where the primary star reaches the tip of the red giant branch are discussed as a formation scenario for hot subluminous B-type (sdB)…