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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S237(2), p. 283-291, 2006

DOI: 10.1017/s1743921307001615

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The mass distribution of unstable cores in turbulent magnetized clouds

Journal article published in 2006 by Paolo Padoan ORCID, Åke Nordlund, Alexei G. Kritsuk, Michael L. Norman, Pak Shing Li ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractThe 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 (~10003computational zones). The striking difference between the HD and MHD regimes, predicted by the model, is recovered.

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