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The Stellar IMF from turbulent fragmentationIn this paper they conclude that turbulent fragmentation is unavoidable in super-sonically turbulent molecular clouds, and given the success of the present model to predict the observed shape of the Stellar IMF, they conclude that turbulent fragmentation is essential to the origin of the stellar IMF.
Document ID
20060040410
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Padoan, P.
Nordlund, A.
Date Acquired
August 23, 2013
Publication Date
January 1, 2001
Distribution Limits
Public
Copyright
Other
Keywords
turbulence

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