THE GIANT MOLECULAR CLOUD MONOCEROS R2 .1. SHELL STRUCTURE

We have obtained a 45'' resolution, Nyquist-sampled map in CO J = 1-0 covering approximately a 3-degrees x 3-degrees region of the giant molecular cloud Monoceros R2. The map consists of 167,000 spectra observed with the 15 element focal-plane array system on the FCRAO 14 m telescope. The data reveal that the large-scale structure of Mon R2 is dominated by a approximately 30 pc diameter largely hemispherical shell containing approximately 4 x 10(4) M. of molecular material and expanding at approximately 3-4 km s-1 with symmetry axis roughly along the line of sight. The dynamical timescale of the shell is estimated to be approximately 4 x 10(6) yr, which is consistent with the age of main-sequence stars powering the clusters of reflection nebulae in this region. There is no evidence for a redshifted shell on the far side of the interior ''bubble'' which is largely devoid of molecular material. Distortions of the shell are obvious, suggesting inhomogeneity of the cloud and possible presence of a magnetic field prior to its formation. Dense clumps in Mon R2, including the main core and the GGD 12-15 core, appear to be condensations located on the large shell. The reflection nebulae with their illuminating stars as well as embedded IRAS sources suggest that triggered star formation has taken place over a large part of the Mon R2 shell.