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