53 citations · 104 across the 7 of their papers we have counts for
4 papers · 1 filter
Angular momentum transport in the convection zone of a 3D MHD simulation of a rapidly rotating core-collapse progenitor
Ryota Shimada, Lucy O. McNeill, Vishnu Varma +3
Rotation and magnetic fields in the cores of evolved massive stars in their final phase are thought to play an important role in the subsequent supernova explosion and the formatio…
Mass transfer stability for AM CVn binaries with white dwarf donors
Lucy O. McNeill, Ryosuke Hirai
Double white dwarf binaries (DWDBs) with Helium components are progenitors to AM CVn binary systems. Their Galactic production rate may be given by the number of stably mass transf…
Differential Rotation in a 3D Simulation of Oxygen Shell Burning
Lucy O. McNeill, Bernhard Müller
We study differential rotation in late-stage shell convection in a 3D hydrodynamic simulation of a rapidly rotating helium star with a particular focus on the convectiv…
Stochastic Core Spin-Up in Massive Stars -- Implications of 3D Simulations of Oxygen Shell Burning
L. O. McNeill, B. Müller
It has been suggested based on analytic theory that even in non-rotating supernova progenitors stochastic spin-up by internal gravity waves (IGWs) during the late burning stages ca…