1. Z.A TomaxiEcA and G.E. Suxeria, J. Phys. Chem. 95 , 6905-6908(1991). 2. R.D. Brown, R. Champion, P.S. Elmes, and P.D. Godfrey, J. Am. Chem. Soc. 107 , 4109-4112(1985). 3. Y. Endo and E. Hirota, J. Chem. Phys. 86 , 4319-4326 (1987).Author Institution: Harvard-Smitsonian Center for Astrophysics, and Department of Chemistry, Harvard University; Herzberg Institute of Astrophysics, National Research Council; Division of Applied Sciences, Harvard University; Division of Applied Sciences, Harvard-Smithsonian Center for AstrophysicsOver 300 rotational transitions of the free radicals HCCCO AND DCCCO between 80 and 400 GHz have been observed by millimeter-wave glow discharge spectroscopy. Analysis of ground state energy levels of N=8=40 and Ka=0β3 using the S-reduced asymmetric top effective Humiltonian, including treatment of a reasonant spin-rotation perturbation, confirms the qualitative ab initio result that HCCCO and DCCCO have highly prolate bent chain structures1. However, the rotational constants are reproduced with better precision by removing one hydrogen from the experimental H2βCCCOstructure,2 implying that HCCCO is more bent than predicted. The rotation and spin-rotation constants indicate that the Renner-Teller effect in this system is stronger than in HCCCO13β and the high degree of distortion is evidence for substantial coupling between bending vibration and rotation about the a-axis. Analysis of the moments of inertia of the two isotopomers yield the a-- and b--axis coordinates of the hydrogen atom and a -- and b--axis moments of inertia for the CCCO subunit in the vibrationally averaged structure