Interstellar Turbulence and Star Formation
Symposium A Quarterly Journal In Modern Foreign Literatures (2010)
- DOI: 10.1017/S1743921311000342
- arXiv: 1011.2177
Available from arxiv.org
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Abstract
We provide a brief overview of recent advances and outstanding issues in simulations of interstellar turbulence, including isothermal models for interior structure of molecular clouds and larger-scale multiphase models designed to simulate the formation of molecular clouds. We show how self-organization in highly compressible magnetized turbulence in the multiphase ISM can be exploited in simple numerical models to generate realistic initial conditions for star formation.
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