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Fig. 12

image

Panels A)D): overlay of the CO emission distribution in contours and the emission at 8 μm in grayscale towards G341.220-0.213. Panel A): 13CO(32) line emission in the interval from 43.8 km s-1 to 42.0 km s-1. Contours are from 5 K to 12 K (Tmb) in steps of 1 K. the different symbols mark the position of YSO candidates: stars: MSX sources, triangles: 2MASS sources, crosses: Spitzer sources, diamonds: WISE sources. Panel B): 13CO(21) line emission in the interval from 44.0 km s-1 to 41.9 km s-1. Contours are from 5 K to 11 K (Tmb) in steps of 1 K. Panel C): C18O(21) line emission in the interval from 43.8 km s-1 to 41.9 km s-1. Contours are from 1.5 K to 4 K (Tmb) in steps of 0.5 K. Panel D): 12CO(21) line emission in the interval from 45.7 km s-1 to 44.3 km s-1. Contours are from 9 K to 14 K (Tmb) in steps of 1 K.

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