Magnetically-driven protostellar jets transport sufficient angular momentum outward to prevent massive protostars from reaching critical rotation speeds, with jet strength linked to initial formation conditions producing a variety of final stellar rotation rates.
Bate MR, Tricco TS, Price DJ
2 Pith papers cite this work, alongside 183 external citations. Polarity classification is still indexing.
2
Pith papers citing it
183
external citations · OpenAlex
verdicts
UNVERDICTED 2representative citing papers
Review of MHD numerical methods for star formation, covering discretization techniques, divergence-free constraints, sink particles, and non-ideal effects like diffusion and the Hall effect.
citing papers explorer
-
On the origin of the rotation of massive stars
Magnetically-driven protostellar jets transport sufficient angular momentum outward to prevent massive protostars from reaching critical rotation speeds, with jet strength linked to initial formation conditions producing a variety of final stellar rotation rates.
-
Numerical Methods for Simulating Star Formation
Review of MHD numerical methods for star formation, covering discretization techniques, divergence-free constraints, sink particles, and non-ideal effects like diffusion and the Hall effect.