The nature of turbulence in OMC 1 at the scale of star formation : observations and simulations ,

@inproceedings{Gustafsson2006TheNO,
  title={The nature of turbulence in OMC 1 at the scale of star formation : observations and simulations ,},
  author={Maiken Gustafsson and Axel Brandenburg and J. L. Lemaire and David Field},
  year={2006}
}
Aims. To study turbulence in the Orion Molecular Cloud (OMC1) by co mparing observed and simulated characteristics of the gas m otions. Methods. Using a dataset of vibrationally excited H 2 emission in OMC1 containing radial velocity and brightness which covers scales from 70 AU to 30000 AU, we present the transversal structure f nctions and the scaling of… CONTINUE READING