This webpage is meant to provide background and explanation for an interactive python code developed to model clumpiness in giant molecular clouds.  This project was created for the Spring 2013  Astronomy 201b: Interstellar Medium and Star Formation at Harvard University taught by Alyssa Goodman. More information about the class can be found at http://ay201b.wordpress.com/

You may contant George Miller at gfmiller@cfa.harvard.edu with any questions or concerns.


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