Angular Momentum Transfer and Lack of Fragmentation in Self-Gravitating Accretion Flows

@article{Begelman2009AngularMT,
  title={Angular Momentum Transfer and Lack of Fragmentation in Self-Gravitating Accretion Flows},
  author={Mitchell C. Begelman and Isaac Shlosman},
  journal={The Astrophysical Journal},
  year={2009},
  volume={702}
}
Rapid inflows associated with early galaxy formation lead to the accumulation of self-gravitating gas in the centers of proto-galaxies. Such gas accumulations are prone to nonaxisymmetric instabilities, as in the well known Maclaurin sequence of rotating ellipsoids, which are accompanied by a catastrophic loss of angular momentum (J). Self-gravitating gas is also intuitively associated with star formation. However, recent simulations of the infall process display highly turbulent continuous… 

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