The physical properties of the molecular clouds in the arm and interarm region of the inner Galalxy are compared. We used Bell Laboratories Galactic Plane 13CO Survey data and UMSB Galactic Plane 12CO Survey data. The LCO/M of the interarm molecular clouds is much smaller that of arm molecular clouds. Several physical properties, including abundance ratio of molecular clouds in two regions are discussed.
American Astronomical Society Meeting Abstracts #193
- Pub Date:
- January 1999