We investigate the influence of large-scale stellar feedback on the formation of molecular clouds in the Large Magellanic Cloud (LMC). Examining the relationship between HI and 12CO(J=1-0) in supergiant shells (SGSs), we find that the molecular fraction in the total volume occupied by SGSs is not enhanced with respect to the rest of the LMC disk. However, the majority of objects (~70% by mass) are more molecular than their local surroundings, implying that the presence of a supergiant shell does on average have a positive effect on the molecular gas fraction. Averaged over the full SGS sample, our results suggest that ~12-25% of the molecular mass in supergiant shell systems was formed as a direct result of the stellar feedback that created the shells. This corresponds to ~4-11% of the total molecular mass of the galaxy. These figures are an approximate lower limit to the total contribution of stellar feedback to molecular cloud formation in the LMC, and constitute one of the first quantitative measurements of feedback-triggered molecular cloud formation in a galactic system.
@article{arxiv.1211.7119,
title = {Supergiant Shells and Molecular Cloud Formation in the LMC},
author = {J. R. Dawson and N. M. McClure-Griffiths and T. Wong and John M. Dickey and A. Hughes and Y. Fukui and A. Kawamura},
journal= {arXiv preprint arXiv:1211.7119},
year = {2013}
}
Comments
14 pages, 6 figures. Accepted for publication in ApJ