The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey IX: CO Observations of NGC 2976 and NGC 3351
arXiv:1308.6209 · doi:10.1093/mnras/stt1625
Abstract
We present CO \textit{J=32} maps of NGC 2976 and NGC 3351 obtained with the James Clerk Maxwell Telescope (JCMT), both early targets of the JCMT Nearby Galaxy Legacy Survey (NGLS). We combine the present observations with CO \textit{J=10} data and find that the computed CO \textit{J=32} to CO \textit{J=10} line ratio () agrees with values measured in other NGLS field galaxies. We compute the M value and find that it is robust against the value of used. Using \textsc{Hi} data from the The \textsc{Hi} Nearby Galaxy Survey (THINGS) survey, we find a tight correlation between surface density of H and star formation rate density for NGC 3351 when CO \textit{J=32} data are used. Finally, we compare the CO \textit{J=32} intensity with the PAH 8 m surface brightness and find a good correlation in the high surface brightness regions. We extend this study to include all 25 \textit{Spitzer} Infrared Nearby Galaxies Survey (SINGS) galaxies within the NGLS sample and find a tight correlation at large spatial scales. We suggest that both PAH 8 m and CO \textit{J=32} are likely to originate in regions of active star formation.
15 pages, 10 figures Monthly Notices of Royal Astronomical Society 2013
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