Supergiant Shells and Molecular Cloud Formation in the LMC

TL;DR

This study quantifies how stellar feedback from supergiant shells in the LMC influences molecular cloud formation, revealing that a significant portion of molecular gas is likely formed due to this feedback process.

Contribution

It provides the first quantitative measurement of feedback-triggered molecular cloud formation in a galactic system, specifically in the LMC.

Findings

Approximately 12-25% of molecular mass in SGS systems formed due to stellar feedback.

Supergiant shells are associated with a higher molecular fraction than their surroundings.

Feedback contributes at least 4-11% to the galaxy's total molecular mass.

Abstract

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.