Left: CS(2-1) emission toward the MWC 1080 system overlaid on a small adaptive optics K'-band image taken from CFHT (Paper II). The noise is 0.14 Jy beam–1 km s–1. The contours are linearly spaced from 2 to 10 times the noise. The beam, shown at the lower right-hand corner, is 
with a P.A. of –62°. Negative contours, mainly from resolved-out large-scale emission, are not shown here in order to simplify the image. The dotted box indicates the zoomed field of the K'-band image (right) in order to show the distribution of young cluster members more clearly.
with a P.A. of –62°. Negative contours, mainly from resolved-out large-scale emission, are not shown here in order to simplify the image. The dotted box indicates the zoomed field of the K'-band image (right) in order to show the distribution of young cluster members more clearly.