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2010MNRAS.406.1350F - Mon. Not. R. Astron. Soc., 406, 1350-1357 (2010/August-1)
The structure of molecular clouds - II. Column density and mass distributions.
FROEBRICH D. and ROWLES J.
Abstract (from CDS):
We find that the low column density and turbulence-dominated part of the clouds can be well fitted by a lognormal distribution. However, above a universal extinction threshold of 6.0±1.5mag AV there is excess material compared to the lognormal distribution in all investigated clouds. This material represents the part of the cloud that is currently involved in star formation, and thus dominated by gravity. Its contribution to the total mass of the clouds ranges over two orders of magnitude from 0.1 to 10 per cent. This implies that our clouds sample various stages in the evolution of GMCs. Furthermore, we find that the column density and mass distributions are extremely similar between clouds if we analyse only the high-extinction material. On the other hand, there are significant differences between the distributions if only the low-extinction, turbulence-dominated regions are considered. This shows that the turbulent properties differ between clouds depending on their environment. However, no significant influence on the predominant mode of star formation (clustered or isolated) could be found. Furthermore, the fraction of the cloud actively involved in star formation is only governed by gravity, with the column density and mass distributions not significantly altered by local feedback processes.
Abstract Copyright: © 2010 The Authors. Journal compilation © 2010 RAS
Journal keyword(s): stars: formation - ISM: clouds - dust, extinction - ISM: structure
Simbad objects: 21
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