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Radiation-hydrodynamic simulations of the formation of orion-like star clusters. II. the initial mass function from winds, turbulence, and radiation

CollectionsANU Research Publications
Date published: 2012
Type: Journal article
URI: http://hdl.handle.net/1885/152125
Source: The Astrophysical Journal
DOI: 10.1088/0004-637X/754/1/71
Access Rights: Open Access

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