COMETARY GLOBULES IN THE SOUTHEAST QUADRANT OF THE ROSETTE NEBULA

We present a study of newly identified cometary globules in the southeast quadrant of the Rosette nebula using the J = 1-0 transition of carbon monoxide. The globules are found to be blueshifted by about 6 km s-1 with respect to the adjacent Rosette molecular cloud. The masses of the globules vary from 50 to 300 M., and their sizes are between 1 and 3 pc. Two of the globules have cometary morphology and show velocity gradients of approximately 1.5 km s-1 pc-1 along their symmetry axes. These globules are associated with the IRAS sources 06314+0421, X0632+043, 06322+0427, and 06327+0423 which coincide with local maxima in the (CO)-C-13 emission. The derived physical parameters of the globules are found to be consistent with those predicted by recent theoretical models of photoevaporating cometary clouds. We suggest that star formation induced by radiation driven implosion has occurred.