Modeling mass functions of clumps formed during the early MC evolution
Astrophysics of Galaxies
2012-08-15 v1 Solar and Stellar Astrophysics
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.
Keywords
Cite
@article{arxiv.1208.2799,
title = {Modeling mass functions of clumps formed during the early MC evolution},
author = {Todor V. Veltchev and Sava Donkov},
journal= {arXiv preprint arXiv:1208.2799},
year = {2012}
}
Comments
A poster report, presented at the conference Galactic Scale Star Formation: Observation meets theory, Heidelberg, July 30 - August 3, 2012; 5 pages, 3 figures