Modeling mass functions of clumps formed during the early MC evolution
arXiv:1208.2799
Abstract
The statistical approach for description of molecular cloud substructure, proposed by Donkov, Veltchev and Klessen (2011, 2012), allows for alternative models, operating with different type of objects: an ensemble of clumps or a larger cloudlet. We demonstrate briefly the predictive power of both models, applied to molecular emission and dust extinction studies of Galactic clouds.
A poster report, presented at the conference Galactic Scale Star Formation: Observation meets theory, Heidelberg, July 30 - August 3, 2012; 5 pages, 3 figures