Molecular gas dynamics in the Rosette Nebula

Details Molecular gas dynamics in the Rosette Nebula Molecular gas dynamics in the Rosette Nebula

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..251..125m&link_type=abstract

Organic Matter in Space, Proceedings of the International Astronomical Union, IAU Symposium, Volume 251, p. 125-126

Astronomy and Astrophysics

Astronomy

Ism: Molecules, Ism: Kinematics And Dynamics, Instrumentation: Detectors

Scientific paper

We 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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