72 citations · 181 across the 3 of their papers we have counts for
3 papers
Constructing stable 3D hydrodynamical models of giant stars
Sebastian T. Ohlmann, Friedrich K. Roepke, Rüdiger Pakmor +1
Hydrodynamical simulations of stellar interactions require stable models of stars as initial conditions. Such initial models, however, are difficult to construct for giant stars be…
Magnetic Field Amplification During the Common Envelope Phase
Sebastian T. Ohlmann, Friedrich K. Roepke, Ruediger Pakmor +2
During the common envelope (CE) phase, a giant star in a binary system overflows its Roche lobe and unstable mass transfer leads to a spiral-in of the companion, resulting in a clo…
The white dwarf's carbon fraction as a secondary parameter of Type Ia supernovae
Sebastian T. Ohlmann, Markus Kromer, Michael Fink +4
Binary stellar evolution calculations predict that Chandrasekhar-mass carbon/oxygen white dwarfs (WDs) show a radially varying profile for the composition with a carbon depleted co…