Abstract
AbstractWe present observations of the Rosette Nebula and its near environment in the CO 3–2 transition obtained with an angular resolution of 20″. The gas dynamics of the region are complex; we find (1) a ring of gas expanding at about 20 km s−1, (2) a number of collimated outflow sources, and (3) a chain of dust clumps having a velocity gradient along its length.
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