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A constrained-transport magnetohydrodynamics algorithm with near-spectral resolution
Jason Maron, Mordecai-Mark Mac Low, Jeffrey Oishi
Numerical simulations including magnetic fields have become important in many fields of astrophysics. Evolution of magnetic fields by the constrained transport algorithm preserves…
Supplementary Information for ``Rapid planetesimal formation in turbulent circumstellar discs''
Anders Johansen, Jeffrey S. Oishi, Mordecai-Mark Mac Low +3
This document contains refereed supplementary information for the paper ``Rapid planetesimal formation in turbulent circumstellar discs''. It contains 15 sections (\S1.1 -- \S1.15)…
Rapid planetesimal formation in turbulent circumstellar discs
Anders Johansen, Jeffrey S. Oishi, Mordecai-Mark Mac Low +3
The initial stages of planet formation in circumstellar gas discs proceed via dust grains that collide and build up larger and larger bodies (Safronov 1969). How this process conti…
Turbulent Torques on Protoplanets in a Dead Zone
Jeffrey S. Oishi, Mordecai-Mark Mac Low, Kristen Menou
Migration of protoplanets in their gaseous host disks may be largely responsible for the observed orbital distribution of extrasolar planets. Recent simulations have shown that the…