Physics
Scientific paper
Apr 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..384...71h&link_type=abstract
14th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun ASP Conference Series, Vol. 384, proceedings of the conferen
Physics
Scientific paper
Recent developments in dynamical theories of star formation may be essential to understanding the origin of stellar initial mass function. In this article I focus on what dynamical models imply for the formation of brown dwarfs. I also consider how global collapse of molecular clouds might help explain how star clusters form (the dominant mode of star formation). Finally, I suggest that a dynamical picture of molecular cloud core formation naturally results in the frequent production of binary or multiple star systems.
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