Abstract
We present observations of the Rosette Nebula and its near environment in the CO 32 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 s1, (2) a number of collimated outflow sources, and (3) a chain of dust clumps having a velocity gradient along its length. © 2008 International Astronomical Union.
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Matthews, H. E., & Dent, W. R. F. (2008). Molecular gas dynamics in the Rosette Nebula. In Proceedings of the International Astronomical Union (Vol. 4, pp. 125–126). Cambridge University Press. https://doi.org/10.1017/S1743921308021340
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