165 citations · 1.4k across the 30 of their papers we have counts for
31 papers
Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
G. Leidi, A. Holas, K. Vitovsky +12
We present PHLEGETHON, a fully compressible, Eulerian magnetohydrodynamic (MHD) code designed for multidimensional simulations in stellar astrophysics. The code uses a time-explici…
On the Geometry of the Near-Core Magnetic Field in Massive Stars
Rathish P. Ratnasingam, Philipp V. F. Edelmann, Dominic M. Bowman +1
It is well-known that the cores of massive stars sustain a stellar dynamo with a complex magnetic field configuration. However, the same cannot be said for the field's strength and…
Effect of Rotation on Wave Mixing in Intermediate Mass Stars
A. Varghese, R. P. Ratnasingam, R. Vanon +3
Internal gravity waves (IGWs) are likely to cause mixing in stellar interiors. Studies show that the mixing by these waves changes drastically across age and mass (Varghese et al.…
Turbulent dynamo action and its effects on the mixing at the convective boundary of an idealized oxygen-burning shell
G. Leidi, R. Andrassy, J. Higl +2
Convection is one of the most important mixing processes in stellar interiors. Hydrodynamic mass entrainment can bring fresh fuel from neighboring stable layers into a convection z…
Multidimensional Simulations of Core Convection
Daniel Lecoanet, Philipp V. F. Edelmann
The cores of main sequence intermediate- and high-mass stars are convective. Mixing at the radiative-convective boundary, waves excited by the convection, and magnetic fields gener…
Three-Dimensional Simulations of Massive Stars: II. Age Dependence
R. Vanon, P. V. F. Edelmann, R. P. Ratnasingam +2
We present 3D full star simulations, reaching up to 90% of the total stellar radius, for three stars of different ages (ZAMS, midMS and TAMS). A comparison with several…