Study of the molecular gas towards the N11 region in the Large Magellanic Cloud

Abstract

We study three subregions in the HII region N11 which is located at the northeast side of the Large Magellanic Cloud (LMC). We used ${}^{12}$CO and ${}^{13}$CO J=3--2 data observed with the Atacama Submillimeter Telescope Experiment (ASTE) with an angular and spectral resolution of 22${}^{\prime \prime }$ and 0.11 km s${}^{-1}$ respectively. From the ${}^{12}$CO J=3--2 and ${}^{13}$CO J=3--2 integrated maps we estimated, assuming local thermodynamic equilibrium (LTE), masses in about $10^4$ M${}_{\odot }$ for the molecular clouds associated with each subregion. Additionally, from the mentioned maps we study the ${}^{12}$CO /${}^{13}$CO integrated ratios for each subregion, obtaining values between 8 and 10.