Article contents
The mass distribution of unstable cores in turbulent magnetized clouds
Published online by Cambridge University Press: 01 August 2006
Abstract
The predictions of the Padoan and Nordlund IMF model are tested using the largest simulations of supersonic hydrodynamic (HD) and magneto-hydrodynamic (MHD) turbulence to date (~10003 computational zones). The striking difference between the HD and MHD regimes, predicted by the model, is recovered.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 283 - 291
- Copyright
- Copyright © International Astronomical Union 2007
References
- 1
- Cited by